| NGC 753 | |
|---|---|
 PanSTARRS image of NGC 753. | |
| Observation data (J2000 epoch) | |
| Constellation | Andromeda |
| Right ascension | 01h 57m 42.2s[1] |
| Declination | 35° 54′ 58″[1] |
| Redshift | 0.016355[1] |
| Heliocentric radial velocity | 4903 km/s[1] |
| Distance | 220 Mly (67 Mpc)[2] |
| Group or cluster | Abell 262 |
| Apparent magnitude (V) | 12.97[1] |
| Characteristics | |
| Type | SAB(rs)bc[1] |
| Size | ~150,000 ly (46 kpc) (estimated)[1] |
| Apparent size (V) | 2.5 x 1.9[1] |
| Other designations | |
| MCG 6-5-66, PGC 7387, UGC 1437[1] | |
Preview warning: Page using Template:Infobox galaxy with unknown parameter "upright"
NGC 753 is a spiral galaxy[3] located 220 million light-years away[2] in the constellation Andromeda. The galaxy was discovered by astronomer by Heinrich d'Arrest on September 16, 1865[4] and is a member of Abell 262.[5][6][7][8][9][10]
NGC 753 has roughly 2-3 times more mass than the Milky Way[5] and is classified as a radio galaxy.[11][12][13]
- ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 753. Retrieved 2019-01-03.
- ^ a b Pilyugin, L. S.; Grebel, E. K.; Kniazev, A. Y. (2014). "The Abundance Properties of Nearby Late-type Galaxies. I. The Data". The Astronomical Journal. 147 (6): 131. arXiv:1403.5461. Bibcode:2014AJ....147..131P. doi:10.1088/0004-6256/147/6/131. ISSN 1538-3881. S2CID 119239041.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-01-03.
- ^ "New General Catalog Objects: NGC 750 - 799". cseligman.com. Retrieved 2019-01-03.
- ^ a b Henry, R. B. C.; Balkowski, C.; Cayatte, V.; Edmunds, M. G.; Pagel, B. E. J. (1996-12-01). "The effects of cluster environment on the chemical evolution of galaxies. III. NGC 753". Monthly Notices of the Royal Astronomical Society. 283 (2): 635–647. Bibcode:1996MNRAS.283..635H. doi:10.1093/mnras/283.2.635. ISSN 0035-8711.
- ^ Giuricin, G.; Marinoni, C.; Ceriani, L.; Pisani, A. (November 2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". The Astrophysical Journal. 543 (1): 178–194. arXiv:astro-ph/0001140. Bibcode:2000ApJ...543..178G. doi:10.1086/317070. ISSN 0004-637X. S2CID 9618325.
- ^ Garcia, A. M. (1993-07-01). "General study of group membership. II - Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47–90. Bibcode:1993A&AS..100...47G. ISSN 0365-0138.
- ^ Fouque, P.; Gourgoulhon, E.; Chamaraux, P.; Paturel, G. (1992-05-01). "Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members". Astronomy and Astrophysics Supplement Series. 93: 211–233. Bibcode:1992A&AS...93..211F. ISSN 0365-0138.
- ^ "NGC 753". sim-id. Retrieved 2019-01-03.
- ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2019-01-03.
- ^ Righetti, G.; Giovannini, G.; Feretti, L. (1988-04-01). "WSRT observations at 327 MHz of the cluster A262". Astronomy and Astrophysics Supplement Series. 73: 173–179. Bibcode:1988A&AS...73..173R. ISSN 0365-0138.
- ^ Zhao, Jun-Hui; Burns, Jack O.; Owen, Frazer N. (1989-07-01). "A 20 CM VLA survey of Abell clusters of galaxies. I - Distance class of not greater than 3 clusters". The Astronomical Journal. 98: 64–107. Bibcode:1989AJ.....98...64Z. doi:10.1086/115128. ISSN 0004-6256.
- ^ Miller, Neal A.; Owen, Frazer N. (2001-06-01). "The Radio Galaxy Populations of Nearby Northern Abell Clusters". The Astrophysical Journal Supplement Series. 134 (2): 355–383. arXiv:astro-ph/0101114. Bibcode:2001ApJS..134..355M. doi:10.1086/320857. ISSN 0067-0049. S2CID 119052072.