NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: Mon Aug 19 10:54:45 2019 PDT
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Classifications for NGC 7814

35 Classifications found in NED

   NGC 7814


Published NED Homogenized
Classification Reference Code Classification Flag Bandpass Region Notes
Hierarchy
GR
1992A&AS...93..211F
 i  Group member, radial-velocity confirmed
...
Optical
Environment
see NGC 7814 GROUP
GM
1984TarOT..73....1V
 i  Group member
...
Optical
Environment
see VNK.002
Kinematics
HI line width
1980A&A....88...32B
 i  HI line width
...
Radio
Galaxy
From HyperLEDA (Sept. 2010):
log(w) = 2.689; [w = 488 km/s]
5: HI line width measured at 50% of maximum
HI line width
1980A&A....88...32B
 i  HI line width
...
Radio
Galaxy
From HyperLEDA (Sept. 2010):
log(w) = 2.707; [w = 509 km/s]
4: HI line width measured at 40% of maximum
HI line width
1980A&A....88...32B
 i  HI line width
...
Radio
Galaxy
From HyperLEDA (Sept. 2010):
log(w) = 2.777; [w = 598 km/s]
1: HI line width measured at 20% of maximum
HI line width
1980AJ.....85.1312K
 i  HI line width
...
Radio
Galaxy
From HyperLEDA (Sept. 2010):
log(w) = 2.665; [w = 462 km/s]
5: HI line width measured at 50% of maximum
HI line width
1983A&AS...51..331B
 i  HI line width
...
Radio
Galaxy
From HyperLEDA (Sept. 2010):
log(w) = 2.660; [w = 457 km/s]
1: HI line width measured at 20% of maximum
HI line width
2005ApJS..160..149S
 i  HI line width
...
Radio
Galaxy
From HyperLEDA (Sept. 2010):
log(w) = 2.671; [w = 468 km/s]
5: HI line width measured at 50% of maximum
HI line width
1987AJ.....94..883B
 i  HI line width
...
Radio
Galaxy
From HyperLEDA (Sept. 2010):
log(w) = 2.667; [w = 464 km/s]
5: HI line width measured at 50% of maximum
HI line width
2005ApJS..160..149S
 i  HI line width
...
Radio
Galaxy
From HyperLEDA (Sept. 2010):
log(w) = 2.681; [w = 479 km/s]
1: HI line width measured at 20% of maximum
Luminosity Class
2.0
1991RC3.9.C...0000d
 i  LC I-II
...
Optical
Galaxy
...
Galaxy Morphology
SA(s)ab: edge-on
1991RC3.9.C...0000d
 i  SA(s)ab? edge-on
...
Optical
Galaxy
Code: [.SAS2*/]
S(ab)
1981RSA...C...0000S
 i  Sab?
...
Optical
Galaxy
Code: [S 2U]
Sa-b
1973UGC...C...0000N
 i  Sab
...
Optical
Galaxy
...
2s
1975SoByu..47...43A
 i  structured nuclear region
...
Optical
Galaxy
...
thin disk
1994CAG1..B...0000S
 i  thin disk
...
Optical
Galaxy
...
silhouetted dust lanes
1994CAG1..B...0000S
 i  silhouetted dust lanes
...
Optical
Galaxy
...
parallel dust lanes
1994CAG1..B...0000S
 i  parallel dust lanes
...
Optical
Galaxy
...
edge-on
1994CAG1..B...0000S
 i  edge-on
...
Optical
Galaxy
...
not lopsided
2005A&A...438..507B
 i  not lopsided
...
Near-Infrared
Galaxy
A1 = 0.017; A2 = 0.040
very bright central bulge
1964RC1...C...0000d
 i  very bright central bulge
...
Optical
Galaxy
...
thin dark lane
1964RC1...C...0000d
 i  thin dark lane
...
Optical
Galaxy
...
strong dark lane
1964RC1...C...0000d
 i  strong dark lane
...
Optical
Galaxy
...
secondary layer of dark material
1964RC1...C...0000d
 i  secondary layer of dark material
...
Optical
Galaxy
...
outer bulge
1964RC1...C...0000d
 i  outer bulge
...
Optical
Galaxy
...
edge-on dark lane
1964RC1...C...0000d
 i  edge-on dark lane
...
Optical
Galaxy
...
Distance Indicator
Tully-Fisher
2009ApJS..182..474S
 i  Tully-Fisher
...
Optical
Galaxy
(m-M) = 31.71 +/- 0.4 mag
D = 21.9 Mpc
Tully-Fisher
2011A&A...532A.104N
 i  Tully-Fisher
...
Optical
Galaxy
(m-M) = 30.95 +/- 0.4 mag
D = 15.5 Mpc
Tully-Fisher
2009AJ....138..323T
 i  Tully-Fisher
...
Optical
Galaxy
(m-M) = 31.29 +/- 0.36 mag
D = 18.1 Mpc
Tully-Fisher
2009ApJS..182..474S
 i  Tully-Fisher
...
Optical
Galaxy
(m-M) = 31.69 +/- 0.4 mag
D = 21.8 Mpc
Tully est
1988NBGC.C....0000T
 i  Tully est
...
Optical
Galaxy
(m-M) = 30.9 +/- 0.8 mag
D = 15.1 Mpc
TRGB
2011ApJS..195...18R
 i  TRGB
...
Optical
Galaxy
(m-M) = 30.8 +/- 0.1 mag
D = 14.4 Mpc
Sosies
2002A&A...393...57T
 i  Sosies
...
Optical
Galaxy
(m-M) = 31.26 +/- 0.13 mag
D = 17.9 Mpc
SBF
2001ApJ...546..681T
 i  SBF
...
Optical
Galaxy
(m-M) = 30.6 +/- 0.14 mag
D = 13.2 Mpc
SBF
2003ApJ...583..712J
 i  SBF
...
Optical
Galaxy
(m-M) = 30.44 +/- 0.14 mag
D = 12.2 Mpc


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