| NGC 4513 | |
|---|---|
 SDSS image of NGC 4513. | |
| Observation data (J2000 epoch) | |
| Constellation | Draco |
| Right ascension | 12h 32m 01.5s[1] |
| Declination | 66° 19′ 57″[1] |
| Redshift | 0.007685[1] |
| Heliocentric radial velocity | 2304 km/s[1] |
| Distance | 110 Mly (33 Mpc)[1] |
| Group or cluster | NGC 4256 Group |
| Apparent magnitude (V) | 13.7[1] |
| Characteristics | |
| Type | (R)SA0^0[1] |
| Size | ~55,000 ly (17 kpc) (estimated)[1] |
| Apparent size (V) | 1.21 x 0.88[1] |
| Other designations | |
| CGCG 315-42, MCG 11-15-59, PGC 41527, UGC 7683[1] | |
NGC 4513 is a lenticular galaxy[2][3][4] and a ring galaxy[4][5][3] located about 110 million light-years away[2][3] in the constellation Draco. It was discovered by astronomer Heinrich d'Arrest on October 16, 1866.[6]
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4513. Retrieved 2019-04-08.
- ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-04-10.
- ^ a b c Ilyina, M. A.; Sil'chenko, O. K.; Afanasiev, V. L. (2014-03-01). "Nature of star-forming rings in S0 galaxies". Monthly Notices of the Royal Astronomical Society. 439 (1): 334–341. Bibcode:2014MNRAS.439..334I. doi:10.1093/mnras/stt2441. ISSN 0035-8711.
- ^ a b Sil'chenko, Olga K.; Ilyina, Marina A. (2011-05-16). "Lenticular galaxies with UV-rings". arXiv:1105.3147. Bibcode:2011AstL...37..589I. doi:10.1134/S0320010811090051. S2CID 118164747.
{{cite journal}}: Cite journal requires|journal=(help) - ^ Moss, D.; Mikhailov, E.; Silchenko, O.; Sokoloff, D.; Horellou, C.; Beck, R. (August 2016). "Magnetic fields in ring galaxies". Astronomy & Astrophysics. 592: A44. arXiv:1605.01883. Bibcode:2016A&A...592A..44M. doi:10.1051/0004-6361/201628346. ISSN 0004-6361. S2CID 42667458.
- ^ "New General Catalog Objects: NGC 4500 - 4549". cseligman.com. Retrieved 2019-04-10.