IC 1101

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Galaxy
IC 1101
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The galaxy IC 1101, SDSS section with a side length of 3.5 arc minutes
The galaxy IC 1101, SDSS section with a side length of 3.5 arc minutes
AladinLite
Constellation Virgin
Position
equinoxJ2000.0 , epoch : J2000.0
Right ascension 15 h 10 m 56.1 s
declination + 05 ° 44 ′ 41 ″
Appearance
Morphological type cD; S0-:  
Brightness  (visual) 14.0 mag
Brightness  (B-band) 15.0 mag
Angular expansion 1.2 ′ × 0.6 ′
Position angle 23 °
Surface brightness 13.7 mag / arcmin²
Physical data
Affiliation Abell 2029  
Redshift 0.077947 ± 0.000087  
Radial velocity 23368 ± 26 km / s  
Stroke distance
v rad  / H 0
(1045 ± 73)  ·  10 6  Lj
(320.5 ± 22.4)  Mpc 
history
discovery Edward Swift
Discovery date June 19, 1890
Catalog names
IC  1101 • UGC  9752 • PGC  54167 • CGCG  049-023 • 2MASX  J15105610 + 0544416 •

IC 1101 is the central cD galaxy of the galaxy cluster Abell 2029 . It is one of the largest known galaxies . It is located in the constellation Virgo , right on the border with Serpens , at a distance of about a billion light years. Its effective radius is given as 42 arc seconds, corresponding to about 50 kpc (150,000 light years). It is surrounded by a diffuse halo that can be traced from the galaxy for up to 300 arc seconds, i.e. has a diameter of about 900 kpc. However, this halo is not assigned to the galaxy itself, but rather to the galaxy cluster as a so-called intra-cluster light .

The object was discovered on June 19, 1890 by Edward D. Swift .

literature

  • Uson, Juan M .; Boughn, Stephen P .; Kuhn, Jeffrey R .: "The central galaxy in Abell 2029 - an old supergiant"; Science 250, pp. 539f. (1990)
  • Clarke, TE; Blanton, Elizabeth L .; Sarazin, Craig L .: "The Complex Cooling Core of A2029: Radio and X-Ray Interactions"; The Astrophysical Journal 616 (1), pp. 178-191 (2004)

Individual evidence

  1. a b c NASA / IPAC EXTRAGALACTIC DATABASE
  2. a b c d e f SEDS : IC 1101
  3. ^ Fisher, Illingworth & Franx (1995), ApJ 438, 539
  4. Uson, Boughn & Kuhn (1991), ApJ 369, 46
  5. P. Patel et al. (2006), MNRAS 370, 851
  6. Seligman