Astronomy:NGC 679
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Short description: Galaxy in the constellation Andromeda
NGC 679 | |
---|---|
2MASS image of NGC 679. | |
Observation data (J2000 epoch) | |
Constellation | Andromeda |
Right ascension | 01h 49m 43.8s[1] |
Declination | 35° 47′ 08″[1] |
Redshift | 0.016842[1] |
Helio radial velocity | 5049 km/s[1] |
Distance | 213 Mly (65.4 Mpc)[1] |
Group or cluster | Abell 262 |
Apparent magnitude (V) | 13.33[1] |
Characteristics | |
Type | E,[2] S0^-[1] |
Size | ~106,000 ly (32.4 kpc) (estimated)[1] |
Apparent size (V) | 2.1 x 2.1[1] |
Other designations | |
CGCG 522-15, MCG 6-5-12, PGC 6711, UGC 1283[1] |
NGC 679 is an elliptical[3][4][5] or a lenticular galaxy[6][4][5] located 210 million light-years away[6] in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 13, 1784[7] and is a member of Abell 262.[8][9][10][11][12]
It is also a radio galaxy.[13]
Dust Disk
NGC 679 hosts a nearly face-on disk of dust with a diameter of ~9,800 ly (3 kpc).[3]
See also
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 "NASA/IPAC Extragalactic Database". Results for NGC 679. http://nedwww.ipac.caltech.edu/.
- ↑ "HyperLeda Database". Results for NGC 679. http://leda.univ-lyon1.fr/.
- ↑ 3.0 3.1 Wegner, G. A.; Corsini, E. M.; Thomas, J.; Saglia, R. P.; Bender, R.; Pu, S. B. (2012). "Further Evidence for Large Central Mass-to-light Ratios in Early-type Galaxies: The Case of Ellipticals and Lenticulars in the A262 Cluster" (in en). The Astronomical Journal 144 (3): 78. doi:10.1088/0004-6256/144/3/78. ISSN 1538-3881. Bibcode: 2012AJ....144...78W. http://stacks.iop.org/1538-3881/144/i=3/a=78.
- ↑ 4.0 4.1 "HyperLeda -object description". http://leda.univ-lyon1.fr/ledacat.cgi?o=NGC%20679.
- ↑ 5.0 5.1 "NGC 0679". http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC+0679&QueryType=ned.
- ↑ 6.0 6.1 "Your NED Search Results". http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+679&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES.
- ↑ "New General Catalog Objects: NGC 650 - 699" (in en-US). http://cseligman.com/text/atlas/ngc6a.htm#679.
- ↑ P., Fouque; E., Gourgoulhon; P., Chamaraux; G., Paturel (May 1992). "Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members" (in en). Astronomy and Astrophysics Supplement Series 93: 211. ISSN 0365-0138. Bibcode: 1992A&AS...93..211F.
- ↑ M., Garcia, A. (July 1993). "General study of group membership. II - Determination of nearby groups" (in en). Astronomy and Astrophysics Supplement Series 100: 47. ISSN 0365-0138. Bibcode: 1993A&AS..100...47G.
- ↑ Giuricin, Giuliano; Marinoni, Christian; Ceriani, Lorenzo; Pisani, Armando (November 2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups" (in en). The Astrophysical Journal 543 (1): 178–194. doi:10.1086/317070. ISSN 0004-637X. Bibcode: 2000ApJ...543..178G. http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:astro-ph/0001140.
- ↑ "Detailed Object Classifications". http://ned.ipac.caltech.edu/cgi-bin/NEDatt?objname=NGC+0679.
- ↑ "NGC 679". http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC+++679&NbIdent=query_hlinks&Coord=01+49+43.794+35+47+08.39&parents=5&submit=parents&siblings=164&hlinksdisplay=h_all.
- ↑ G., Righetti; G., Giovannini; L., Feretti (April 1988). "WSRT observations at 327 MHz of the cluster A262" (in en). Astronomy and Astrophysics Supplement Series 73: 173. ISSN 0365-0138. Bibcode: 1988A&AS...73..173R.
External links
- NGC 679 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Original source: https://en.wikipedia.org/wiki/NGC 679.
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