NGC474 Galaxy in Pisces

DATE 31 Oct 2013
TELESCOPE OPTICS 508 mm mirror f.4 . effective f4.6 with paracorr2. ccd Kodak KAF8300 3326 x 2504px 5.4 x 5.4µm
EXPOSURE binning 2: composite image, 28 min
IMAGE SIZE (ARCMIN) 24
LIGHT TRAVEL TIME (Derived Redshift. Millions Light Years) NGC474 = 89
NGC470 = 92
2MASX J01203953+0325416 = 958
2MASX J01192575+0326531 = 589
[HB89] 0117+031 NED02 = 9,833
[HB89] 0117+031 NED01 = 9,141
MAGNITUDE NGC474 = 12.37
NGC470 = 12.53
2MASX J01203953+0325416 = 17.0
2MASX J01192575+0326531 = n/a
[HB89] 0117+031 NED02 = 19.9
[HB89] 0117+031 NED01 = 18.2
POSITION RA-DEC J2000 NGC474 = 01:20:06.70 +03:24:55.0
NGC470 = 01:19:44.80 +03:24:36.0
2MASX J01203953+0325416 = 01:20:39.50 +03:25:41.0
2MASX J01192575+0326531 = 01:19:25.70 +03:26:53.0
[HB89] 0117+031 NED02 = 01:19:49.10 +03:23:32.0
[HB89] 0117+031 NED01 = 01:19:48.30 +03:23:20.0
POSITION ANGLE:  
Rotation Velocity km/s NGC474 = n/a.
NGC470 = 200
Size (Light Years) NGC474 = 293,000 (POSS1 103a-O)
NGC470 = 121,000 (POSS1 103a-O)
DETAILS NGC474 is a ringed spiral which is 'gas poor', meaning that it has probably lost it's gases in an encounter with another galaxy. The peculiar geometry of this galaxy also indicates a three dimensional morphology rather than a disc. NGC470 is also a spiral that may be accreting material from NGC474. The supernova SN 1966H was discovered in this region. [HB89] 0117+031 NED02 and [HB89] 0117+031 NED01 are QSOs

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