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Results for object MESSIER 082 (m82)

  • Overview
  • Cross-IDs (87)
  • Coordinates (80)
  • Redshifts (41)
  • Distances (21)
  • Classifications (40)
  • Galactic Extinctions
  • Notes (36)
  • Diameters (9)
  • Photometry & SED (400)
  • Spectra (28)
  • Images (111)
  • References (2315)
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Results from query to NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This work was (partially) supported by the US National Virtual Observatory development project, which is funded by the National Science Foundation under cooperative agreement AST0122449 with The Johns Hopkins University. Main information about object (Cone Search results) A sequential object number applicable to this list only. NED preferred name for the object Right Ascension in degrees (Equatorial J2000.0) Declination in degrees (Equatorial J2000.0) NED's Preferred Object Type: G,GPair,GTrpl,GGroup,GClstr,QSO,AbLS,RadioS,IrS,EmLS,UvES,XrayS,SN Velocity in km/sec, based on known heliocentric redshift Heliocentric redshift for the object, if it exists in NED Quality flag for known heliocentric redshift NED's Basic Data magnitude and filter, generally in an optical band. Angular separation of the object coordinates and the search coordinate. Number of literature references in NED Number of catalog notes in NED Number of photometric data points stored by NED for the object Number of position data points stored by NED for the object Number of redshift data points stored by NED for the object. Number of diameter data points stored by NED for the object. Number of NED associations for the object.
1 MESSIER 082 148.96969 69.67938 G 203 0.000677 2315 36 400 80 41 9 0
Table of the NED's names for the object Valid NED name for the object NED's Object Type, associated with this name
MESSIER 082 G
NGC 3034 G
UGC 05322 G
ARP 337 G
CGCG 333-008 G
CGCG 0951.7+6955 G
MCG +12-10-011 G
2MFGC 07685 G
PRC D-13 G
3C 231 RadioS
4C +69.12 RadioS
2MASX J09555243+6940469 IrS
SDSS J095551.73+694048.6 G
IRAS 09517+6954 IrS
IRAS F09517+6954 IrS
AKARI J0955536+694050 IrS
KTG 28B G
KPG 218B G
LDCE 0842 NED005 G
HDCE 0552 NED003 G
PGC1 0028630 NED002 G
Cigar Galaxy G
PGC 028655 G
RBS 0809 G
UZC J095557.0+694110 G
11HUGS 167 G
87GB 095143.5+695452 RadioS
87GB[BWE91] 0951+6954 RadioS
[WB92] 0951+6954 RadioS
NVSS J095551+694046 RadioS
VLSS J0955.8+6940 RadioS
6C B095143.6+695502 RadioS
8C 0951+699 RadioS
UITBOC 1644 VisS
S4 0951+69 RadioS
CLASS J0955+6940 RadioS
DA 277 RadioS
NRAO 0341 RadioS
TXS 0951+699 RadioS
GB6 J0955+6940 RadioS
HIJASS J0955+69 NED02 RadioS
OCARS 0951+699 RadioS
RGB J0955+696 RadioS
WMAP 088 RadioS
WMAP J0955+6936 RadioS
WMAP J095547+6935 RadioS
WMAP J095549+6935 RadioS
NEWPS_5yr_5s 233 RadioS
NEWPS_5yr_5s_15 226 RadioS
QVW5 J095527+6940 RadioS
QVW7 J095540+694120 RadioS
WMAP3-NEWPS-5S 128 RadioS
AFGL 1388 IrS
CXOU J095552.7+694045 XrayS
CXOU J095552.8+694045 XrayS
RX J0955.8+6940 XrayS
1RXS J095550.4+694052 XrayS
2PBC J0955.7+6941 XrayS
SAXWFC J0955.6+6940.6 XrayS
1AXG J095549+6940 XrayS
1H 0950+696A XrayS
1ES 0951+699 XrayS
SWIFT J0956.1+6942 XrayS
2FGL J0955.9+6936 GammaS
1FGL J0956.5+6938 GammaS
TeV J0955+696 GammaS
[KWP81] 0951+69 RadioS
[dML87] 745 G
[SPB93] 116 G
LGG 176:[G93] 012 G
[MHH96] J095550+694041 XrayS
[SPS97] 08 XrayS
NGC 3031:[R97] 01 XrayS
[M98j] 080 NED03 G
[TSA98] J095541.25+693927.31 XrayS
RX J0955.8+6940:[BEV98] 003 G
[DSL2000] 0951+700 RadioS
[HRT2007] J095552+694047 RadioS
[JBB2007] J095552.72+694045.7 RadioS
MESSIER 082:[TOH2007] X-1 XrayS
[LTS2012] F09565+6938 G
NGC 3034:[MGS2012] 01 XrayS
[BTM2013] 0478 XrayS
Table of the Position Data for the object The reference code for the position adopted by NED. Right Ascension in degrees (Equatorial B1950.0) Declination in degrees (Equatorial B1950.0) Right Ascension in sexagesimal units (Equatorial B1950.0) Declination in sexagesimal units (Equatorial B1950.0) Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi-major-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi- minor-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi-axes position angle. Right Ascension in degrees (Equatorial J2000.0) Declination in degrees units (Equatorial J2000.0) Right Ascension in sexagesimal units (Equatorial J2000.0) Declination in sexagesimal units (Equatorial J2000.0) Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi- major-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi- minor-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi-axes position angle. Longitude in decimal degrees (Ecliptic B1950.0) Latitude in degrees (Ecliptic B1950.0) Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi- major-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi- minor-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi-axes position angle. Longitude in decimal degrees (Ecliptic J2000.0) Latitude in degrees (Ecliptic J2000.0) Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi- major-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi- minor-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi-axes position angle. Longitude in decimal degrees (Galactic) Latitude in degrees (Galactic) Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi- major-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi- minor-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi-axes position angle. Longitude in decimal degrees (Super Galactic) Latitude in degrees (Super Galactic) Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi- major-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi- minor-axes ; or, for galaxy pairs, the radius of a circle enclosing the positions of the two galaxies. Position uncertainties in arcseconds given as the 95 percent confidence ellipse semi-axes position angle.
147.933322 69.916577 09h51m43.997s +69d54m59.68s 5.00E-01 5.00E-01 0 148.969687 69.679383 09h55m52.725s +69d40m45.78s 5.00E-01 5.00E-01 0 118.277833 52.102841 5.00E-01 5.00E-01 0 118.980860 52.108301 5.00E-01 5.00E-01 0 141.409498 40.567579 5.00E-01 5.00E-01 0 40.722287 1.054520 5.00E-01 5.00E-01 0
Redshift Independent Distances for the object Statistical method for calculation distance for the object Distance Modulus in mag. Metric Distance in Mpc. Number of measurements for this object
Mean 27.88 3.835 21
Std. Dev. 0.40 0.730 21
Min. 26.90 2.400 21
Max. 28.70 5.500 21
Median 27.84 3.700 21
Classifications (Types, Attributes) for the object Type of the classification for the object Classification as published NED Homogenized Classification NED flag for Classification The reference code
Hierarchy PP Pair member (points to parent)
Kinematics HI line width HI line width
Galaxy Morphology I0 edge-on I0 edge-on
Radio Morphology I FR I
Distance Indicator Tully est Tully est
Table of the Derived Values for the object The heliocentric radial velocity in km/sec The uncertainty on the Heliocentric radial velocity in km/sec, when known. The reference code for the Heliocentric velocity The heliocentric radial velocity, corrected to the Local Standard of Rest (Kinematic) in km/sec The uncertainty on the LSR radial velocity in km/sec, when known. The reference code for the LSR velocity The Galactocentric (GSR) radial velocity in km/sec, based on heliocentric redshift The uncertainty on the Galactocentric (GSR) radial velocity in km/sec, when known. The reference code for the Galactocentric velocity Radial velocity, derived from the heliocentric redshift, in the Local Group reference frame. The uncertainty on the radial velocity in the Local Group reference frame. The reference code for the radial velocity in the Local Group reference frame. Radial velocity , derived from the heliocentric redshift, in the Cosmic Microwave Background reference frame. The uncertainty on the radial velocity in the Cosmic Microwave Background reference frame. The reference code for the radial velocity in the Cosmic Microwave Background reference frame. Radial velocity, based on the local velocity field model, using only the term for the influence of the Virgo Cluster. The uncertainty on the radial velocity, based on the local velocity field model, using only the term for the influence of the Virgo Cluster. The reference code for the radial velocity, based on the local velocity field model, using only the term for the influence of the Virgo Cluster. Radial velocity, based on the local velocity field model, using the terms for the influence of Virgo Cluster and the Great Attractor only. The uncertainty on the radial velocity, based on the local velocity field model, using only the terms for the influence of the Virgo Cluster and the Great Attractor. The reference code for the radial velocity, based on the local velocity field model, using only the terms for the influence of the Virgo Cluster and the Great Attractor. Radial velocity, based on the local velocity field model, using the terms for the influence of Virgo Cluster, the Great Attractor, and the Shapley Supercluster. The uncertainty on the radial velocity, based on the local velocity field model, using only the terms for the influence of the Virgo Cluster, the Great Attractor, and the Shapley Supercluster. The reference code for the radial velocity, based on the local velocity field model, using only the terms for the influence of the Virgo Cluster, the Great Attractor, and the Shapley Supercluster. Hubble Flow Distance, calculated from the apparent corrected Galactocentric velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty on the Hubble Flow Distance, calculated from the apparent corrected Galactocentric velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. Distance Modulus, calculated from the apparent corrected Galactocentric velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty on the Distance Modulus, calculated from the apparent corrected Galactocentric velocity. Hubble Flow Distance, calculated from the apparent velocity corrected for the Local Group velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty for Hubble Flow Distance, calculated from the apparent velocity corrected for the Local Group velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. Distance Modulus, calculated from the apparent velocity corrected for the Local Group velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty for Distance Modulus, calculated from the apparent velocity corrected for the Local Group velocity. Hubble Flow Distance, calculated from the apparent velocity corrected for the Cosmic Microwave Background velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty for Hubble Flow Distance, calculated from the apparent velocity corrected for the Cosmic Microwave Background velocity. Distance Modulus, calculated from the apparent velocity corrected for the Cosmic Microwave Background velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty for Distance Modulus, calculated from the apparent velocity corrected for the Cosmic Microwave Background velocity. Hubble Flow Distance, calculated from the apparent velocity corrected for the local velocity field model, using only the term for the influence of the Virgo Cluster, velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty for Hubble Flow Distance, calculated from the apparent velocity corrected for the local velocity field model, using only the term for the influence of the Virgo Cluster, velocity. Distance Modulus, calculated from the apparent velocity corrected for the local velocity field model, using only the term for the influence of the Virgo Cluster, velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty for Distance Modulus, calculated from the apparent velocity corrected for the local velocity field model, using only the term for the influence of the Virgo Cluster, velocity. Hubble Flow Distance, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster and the Great Attractor, velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty for Hubble Flow Distance, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster and the Great Attractor, velocity. Distance Modulus, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster and the Great Attractor, velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty for Distance Modulus, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster and the Great Attractor, velocity. Hubble Flow Distance, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster, the Great Attractor, and the Shapley Supercluster, velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty for Hubble Flow Distance, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster, the Great Attractor, and the Shapley Supercluster, velocity. Distance Modulus, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster, the Great Attractor, and the Shapley Supercluster, velocity assuming H_0 = 67.8 +/- 4.7 km/s/Mpc. The uncertainty for Distance Modulus, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster, the Great Attractor, and the Shapley Supercluster, velocity. Scale at the Hubble Flow Distances in pc/arcsec, calculated from the apparent velocity corrected Galactocentric velocity. Scale at the Hubble Flow Distances in kpc/arcsec, calculated from the apparent velocity corrected Galactocentric velocity. Scale at the Hubble Flow Distances in kpc/arcmin, calculated from the apparent velocity corrected Galactocentric velocity. Scale at the Hubble Flow Distances in Mpc/arcmin, calculated from the apparent velocity corrected Galactocentric velocity. Scale at the Hubble Flow Distances in pc/arcsec, calculated from the apparent velocity corrected for the Local Group velocity. Scale at the Hubble Flow Distances in kpc/arcsec, calculated from the apparent velocity corrected for the Local Group velocity. Scale at the Hubble Flow Distances in kpc/arcmin, calculated from the apparent velocity corrected for the Local Group velocity. Scale at the Hubble Flow Distances in Mpc/arcmin, calculated from the apparent velocity corrected for the Local Group velocity. Scale at the Hubble Flow Distances in pc/arcsec, calculated from the apparent velocity corrected for the Cosmic Microwave Background velocity. Scale at the Hubble Flow Distances in kpc/arcsec, calculated from the apparent velocity corrected for the Cosmic Microwave Background velocity. Scale at the Hubble Flow Distances in kpc/arcmin, calculated from the apparent velocity corrected for the Cosmic Microwave Background velocity. Scale at the Hubble Flow Distances in Mpc/arcmin, calculated from the apparent velocity corrected for the Cosmic Microwave Background velocity. Scale at the Hubble Flow Distances in pc/arcsec, calculated from the apparent velocity corrected for the local velocity field model, using only the term for the influence of the Virgo Cluster velocity. Scale at the Hubble Flow Distances in kpc/arcsec, calculated from the apparent velocity corrected for the local velocity field model, using only the term for the influence of the Virgo Cluster velocity. Scale at the Hubble Flow Distances in kpc/arcmin, calculated from the apparent velocity corrected for the local velocity field model, using only the term for the influence of the Virgo Cluster velocity. Scale at the Hubble Flow Distances in Mpc/arcmin, calculated from the apparent velocity corrected for the local velocity field model, using only the term for the influence of the Virgo Cluster velocity. Scale at the Hubble Flow Distances in pc/arcsec, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster and the Great Attractor velocity. Scale at the Hubble Flow Distances in kpc/arcsec, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster and the Great Attractor velocity. Scale at the Hubble Flow Distances in kpc/arcmin, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster and the Great Attractor velocity. Scale at the Hubble Flow Distances in Mpc/arcmin, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster and the Great Attractor velocity. Scale at the Hubble Flow Distances in pc/arcsec, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster, the Great Attractor, and the Shapley Supercluster velocity. Scale at the Hubble Flow Distances in kpc/arcsec, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster, the Great Attractor, and the Shapley Supercluster velocity. Scale at the Hubble Flow Distances in kpc/arcmin, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster, the Great Attractor, and the Shapley Supercluster velocity. Scale at the Hubble Flow Distances in Mpc/arcmin, calculated from the apparent velocity corrected for the local velocity field model, using only the terms for the influence of the Virgo Cluster, the Great Attractor, and the Shapley Supercluster velocity. Redshift, corrected to the Reference Frame defined by the 3K Microwave Background Radiation. Luminosity Distance based on Concordance Cosmology. Luminosity Distance Modulus based on Concordance Cosmology. Angular-Size Distance based on Concordance Cosmology. Angular-Size Distance Modulus based on Concordance Cosmology. Co-Moving Radial Distance based on Concordance Cosmology. Co-Moving Radial Distance Modulus based on Concordance Cosmology. Co-Moving Tangential Distance based on Concordance Cosmology. Co-Moving Tangential Distance Modulus based on Concordance Cosmology. Co-Moving Volume based on Concordance Cosmology. Light Travel-Time based on Concordance Cosmology. Age at Redshift, corrected to the Reference Frame defined by the 3K Microwave Background Radiation. Age of the Universe . Scale(Cosmology Corrected) in pc/arcsec. Scale(Cosmology Corrected) in kpc/arcsec. Scale(Cosmology Corrected) in kpc/arcmin. Scale(Cosmology Corrected) in Mpc/degree. Surface Brightness Dimming : Flux Density per Unit Area. Surface Brightness Dimming : Magnitude per Unit Area.
203 4 209 41986MNRAS.221.1023K 312 61991RC3.9.C...0000d 348 101996AJ....111..794K 282 71996ApJ...473..576F 415 112000ApJ...529..786M 430 112000ApJ...529..786M 432 112000ApJ...529..786M 4.60 0.3328.320.15 5.13 0.3928.550.16 4.15 0.3128.090.15 6.12 0.4428.930.15 6.35 0.4529.010.15 6.38 0.4529.020.15 22 0.022 1.34 0.08 25 0.025 1.49 0.09 20 0.020 1.21 0.07 30 0.030 1.78 0.11 31 0.031 1.85 0.11 31 0.031 1.86 0.11
Table of the basic data for the object The heliocentric radial velocity in km/sec, based on known heliocentric redshift Quality flag for known heliocentric redshift Velocity's mean error when known Heliocentric redshift Z-value for the object, if it exists in NED Quality flag for known heliocentric redshift Mean error for heliocentric redshift Z-value for the object The reference code Major diameter in arcminutes> Minor diameter in arcminutes> An indicative optical magnitude The morphological type or classification Indicative population count The Galactic reddening E(B-V), in magnitudes , based on the prescription of Schlafly and Finkbeiner(2011ApJ...737..103S) The reference code 2011ApJ...737..103S The Galactic extinction (total absorption in U, lambda= 0.35um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in B, lambda= 0.43um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in V, lambda= 0.54um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in R, lambda= 0.64um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in I, lambda= 0.80um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in u, lambda= 0.36um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in g, lambda= 0.47um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in r, lambda= 0.62um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in i, lambda= 0.75um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in z, lambda= 0.89um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in J, lambda= 1.25um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in H, lambda= 1.66um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in K, lambda= 2.19um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in L, lambda= 3.78um) in magnitudes , based on the prescription of Schlegel et al., recalibrated by Schlafly and Finkbeiner, 2011ApJ...737..103S The Galactic extinction (total absorption in B magnitudes) based on the prescription of Burstein and Heiles The reference code for 1982AJ......87.1165B
202.959522 3.897302 0.00068 0.00001 I0;Sbrst HII 0.138 2011ApJ...737..103S 0.678 0.567 0.429 0.339 0.235 0.663 0.517 0.357 0.266 0.198 0.111 0.070 0.047 0.024 0.120 1982AJ.....87.1165B
The largest diameters in the Visual and Near-Infrared spectra regions, when available Published information for the passband being used Published Apparent Major Axis (2a) [arcsec] Published Apparent Minor Axis (2b) [arcsec] Position Angle in degrees J2000.0 The Reference Level from publication The Reference Code of the used source The NED 19-digit Bibliographic Reference code, URL-encoded Physical Major Axis (2a) [kpc] Physical Minor Axis (2a) [kpc]
POSS1 103a-O 780.00 358.80 65 1973UGC...C...0000N 14.50 6.67
K_s (LGA/2MASS "total") 696.00 222.72 67 2003AJ....125..525J 12.94 4.14
Table of the brightest flux in each of the following spectral regions, when available: Gamma-Ray, X-Ray, Ultraviolet, Visual, Near-Infrared, Mid-Infrared, Far-Infrared, Sub-Millimeter, Millimeter, Radio. The Spectral Region The Band name from publication The Apparent Magnitude or Flux of the source The Reference Code of the used source The NED 19-digit Bibliographic Reference code, URL-encoded The Absolute Magnitude or νLν [W] The Bolometric Magnitude or νLν [L☉(Bolometric)]
Gamma-Ray 0.1-100 GeV (Fermi) 2012ApJS..199...31N 2.15E+33 +/- 2.90E+32 [W] 5.59E+06 +/- 7.53E+05
X-Ray 2-10 keV (BeppoSAX) 2007A%26A...472..705V 8.27E+33 +/- 9.84E+32 [W] 2.15E+07 +/- 2.56E+06
Ultraviolet UV_3150 (m_T) 1995A%26AS..114..527R -18.38 +/- 0.26 [mag] 8.28E+08 +/- 1.41E+08
Visual I 2007ApJ...655..863D 3.09E+36 [W] 8.03E+09
Near-Infrared H_tot (2MASS LGA) 2003AJ....125..525J -22.81 +/- 0.21 [mag] 8.03E+09 +/- 6.76E+08
Mid-Infrared L24 (AKARI) 2010A%26A...514A..14K 8.41E+36 +/- 8.01E+35 [W] 2.19E+10 +/- 2.08E+09
Far-Infrared FIR (IRAS) 1988ApJS...68...91R 1.03E+37 [W] 2.67E+10
Sub-Millimeter 350 microns Herschel 2010A%26A...518L..66R 2.34E+35 +/- 1.97E+34 [W] 6.08E+08 +/- 5.11E+07
Millimeter W (WMAP) 2009ApJS..180..283W 2.15E+32 +/- 6.85E+31 [W] 5.59E+05 +/- 1.78E+05
Radio 22.25 MHz 1980MNRAS.190..903L 1.53E+30 +/- 2.90E+29 [W] 3.97E+03 +/- 7.54E+02
NED's Table of Links to External Archives and Services for this object Resource name/service used to send request Name of related on-line astronomical service . NED's link to related on-line astronomical services that are specific to the survey or catalog associated with the NED names. NED name or coordinates from the crossid list for related astronomical service URL address of related on-line astronomical service .
MESSIER 082
NGC 3034
UGC 05322
CGCG 333-008
CGCG 333-008
MCG +12-10-011
4C +69.12
2MASX J09555243+6940469
SDSS J095551.73+694048.6
SDSS J095551.73+694048.6
SDSS J095551.73+694048.6
SDSS J095551.73+694048.6
SDSS J095551.73+694048.6
SDSS J095551.73+694048.6
IRAS 09517+6954
IRAS F09517+6954
PGC 028655
PGC 028655
Retrieve catalog data for NVSS J095551+694046
TXS 0951+699
GB6 J0955+6940
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40m46s
09h55m52.7s,+69d40'46"
Cross-identifications for
Coordinates for
Preferred Position:    Equatorial J2000.0  ()
Preferred Position of
Reference FrameLongitudeLatitudeLongitudeLatitudeUncertainty Ellipse (arcsec)
Decimal DegreesDecimal DegreesSexagesimalSexagesimalSemimajor (a)Semiminor (b)PA (deg)
RA/Dec Equatorial (J2000.0)
RA/Dec Equatorial (B1950.0)
Galactic
Supergalactic
Ecliptic (J2000.0)
Ecliptic (B1950.0)
Measured Positions for
Redshifts and Derived Quantities for
Preferred Redshift: Z = , H0 = 67.8 km/sec/Mpc, Ωmatter = 0.308, Ωvacuum = 0.692
Quantities Derived from Preferred Redshift for  
Calculated and Corrected Velocities
TypeVelocitiesReference   
V (Heliocentric) ± km/s
V (Kinematic LSR) ± km/s
V (Galactocentric GSR) ± km/s
V (Local Group) ± km/s
V (3K CMB) ± km/s
V (Virgo Infall only) ± km/s
V (Virgo + GA only) ± km/s
V (Virgo + GA + Shapley) ± km/s
Hubble Flow Distance and Distance Modulus (where H0 = 67.8 km/sec/Mpc ± km/sec/Mpc)
TypeDistanceModulus
D (Galactocentric GSR) ± Mpc(m-M) = ± mag
D (Local Group) ± Mpc(m-M) = ± mag
D (3K CMB) ± Mpc(m-M) = ± mag
D (Virgo Infall only) ± Mpc(m-M) = ± mag
D (Virgo + GA only) ± Mpc(m-M) = ± mag
D (Virgo + GA + Shapley) ± Mpc(m-M) = ± mag
Scale at Hubble Flow Distances
TypeValues
Scale (Galactocentric GSR) pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree
Scale (Local Group) pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree
Scale (3K CMB) pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree
Scale (Virgo Infall only) pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree
Scale (Virgo + GA only) pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree
Scale (Virgo + GA + Shapley) pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree
Cosmology-Corrected Quantities [H0 = 67.8 km/sec/Mpc, Ωmatter = 0.308, Ωvacuum = 0.692]
[Redshift as corrected to the ]
TypeValues
Luminosity Distance Mpc (m-M) = mag
Angular-Size Distance (m-M) = mag
Co-Moving Radial Distance (m-M) = mag
Co-Moving Tangential Distance (m-M) = mag
Co-Moving Volume Gpc^3
Light Travel-Time Gyr
Age at Redshift Gyr
Age of Universe Gyr
Scale (Cosmology Corrected) pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree
Surface Brightness DimmingFlux Density per Unit Area = ; Magnitude per Unit Area = mag
Measured Redshifts of
See also Distances.
Redshift-independent Distances for
See also Redshifts.
Classifications for
Galaxy Extinctions for
Notes for
Measured Diameters for
Photometry & SED for
Quick-look Photometry & SED plot for
Quick Look Photometry & Luminosities (brightest flux in each spectral region)
SED Plot
Photometry for
See also Spectra.

Images for object MESSIER 082 (m82)

IRSA
FinderChart
ImagePOSS-II F (North), AAO-SES/SERC-ER (South), Red image
View in IRSA Finderchart

Image Credit: Caltech or AAO/ROE

Preview File Size
KB
Information Lambda
m
Clambda Spectral Region Band FOV 1
arcmin
FOV 2
arcmin
Res.
arcsec
Telescope Refcode  
Preview File Size
KB
Information Lambda
m
Clambda Spectral Region Band FOV 1
arcmin
FOV 2
arcmin
Res.
arcsec
Telescope Refcode  
Literature References for
External Resource Links for
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