IC 1101
Galaxy IC 1101 |
|
---|---|
![]() |
|
The galaxy IC 1101, SDSS section with a side length of 3.5 arc minutes | |
AladinLite | |
Constellation | Virgin |
Position equinox : J2000.0 , 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 .
IC 1101 at 702 nm wavelength (red light)
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)