NGC 935/IC 1801
NGC 935 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Aries |
Right ascension | 02h 28m 11.146s[1] |
Declination | +19° 35′ 56.83″[1] |
Redshift | 0.013807[2] |
Distance | 189 ± 13 Mly (57.8 ± 4.0 Mpc)[3] |
Type | Scd:[3] |
Apparent dimensions (V) | 1.857′ × 1.077′[1] |
Apparent magnitude (V) | 12.5[3] |
Other designations | |
2MASX J02281114+1935568, ADBS J022807+1935, APG 276, IRAS 02253+1922, KPG 68, LEDA 9388, MCG+03-07-015, NGC 935, UGC 1937, VV 238, VV 238a, Z 0225.4+1922, Z 462-16 | |
IC 1801 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Aries |
Right ascension | 02h 28m 12.753s[1] |
Declination | +19° 34′ 59.96″[1] |
Redshift | 0.013233[2] |
Type | SBb:[4] |
Apparent dimensions (V) | 1.517′ × 0.849′[1] |
Apparent magnitude (V) | 14.56[4] |
Other designations | |
2MASX J02281275+1934599, KPG 68b, LEDA 9392, MCG+03-07-016, UGC 1936, VV 238b, Z 462-15, Z 0225.4+1921 | |
NGC 935 and IC 1801 are a pair of interacting galaxies within the Aries constellation. NGC 935 is the northern member of the pair and IC 1801 is the southern.
References
- 1 2 3 4 5 6 Skrutskie, M. F.; et al. (February 2006), "The Two Micron All Sky Survey (2MASS)", The Astronomical Journal 131 (2): 1163–1183, Bibcode:2006AJ....131.1163S, doi:10.1086/498708.
- 1 2 Kochanek, C. S.; et al. (October 2001), "The K-Band Galaxy Luminosity Function", The Astrophysical Journal 560 (2): 566–579, arXiv:astro-ph/0011456, Bibcode:2001ApJ...560..566K, doi:10.1086/322488.
- 1 2 3 "NED results for object NGC 0935", NASA/IPAC Extragalactic Database (NASA), retrieved 2015-10-14.
- 1 2 "NED results for object IC 1801", NASA/IPAC Extragalactic Database (NASA), retrieved 2015-10-14.
External links
- "Arp 276". SIMBAD. Centre de données astronomiques de Strasbourg.
- Image ARP 276
- NGC 935/IC 1801 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Coordinates: 02h 28m 10.9s, +19° 35′ 58″
This article is issued from Wikipedia - version of the Thursday, April 21, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.