By Name | NASA/IPAC Extragalactic Database

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

2332

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

0

148.969687

69.679383

09h55m52.725s

+69d40m45.78s

5.00E-01

0

118.277833

52.102841

5.00E-01

0

118.980860

52.108301

5.00E-01

0

141.409498

40.567579

5.00E-01

0

40.722287

1.054520

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

4

1986MNRAS.221.1023K

312

6

1991RC3.9.C...0000d

348

10

1996AJ....111..794K

282

7

1996ApJ...473..576F

415

11

2000ApJ...529..786M

430

11

2000ApJ...529..786M

432

11

2000ApJ...529..786M

4.60

0.33

28.32

0.15

5.13

0.39

28.55

0.16

4.15

0.31

28.09

0.15

6.12

0.44

28.93

0.15

6.35

0.45

29.01

0.15

6.38

0.45

29.02

0.15

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 Frame	Longitude	Latitude	Longitude	Latitude	Uncertainty Ellipse (arcsec)
	Decimal Degrees	Decimal Degrees	Sexagesimal	Sexagesimal	Semimajor (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
Type	Velocities	Reference
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)
Type	Distance	Modulus
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
Type	Values
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, Ω_matter = 0.308, Ω_vacuum = 0.692]
[Redshift as corrected to the ]
Type	Values
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 Dimming	Flux Density per Unit Area = ; Magnitude per Unit Area = mag

Measured Redshifts of

Images for object MESSIER 082 (m82)

POSS-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

NASA/IPAC Extragalactic Database

Help Detailed Information for a Named Object

Results for object MESSIER 082 (m82)

Images for object MESSIER 082 (m82)

Quick Look Photometry & Luminosities (brightest flux in each spectral region)	SED Plot

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Help Detailed Information for a Named Object

Results for object MESSIER 082 (m82)

Images for object MESSIER 082 (m82)