NGC 3512
| NGC 3512 | |
|---|---|
 NGC 3512 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Leo |
| Right ascension | 11h 04m 02.9449s[1] |
| Declination | +28° 02′ 12.888″[1] |
| Redshift | 0.004580±0.00000200[1] |
| Heliocentric radial velocity | 1,373±1 km/s[1] |
| Distance | 113.50 ± 11.20 Mly (34.800 ± 3.434 Mpc)[2] |
| Group or cluster | NGC 3504 group (LGG 227) |
| Apparent magnitude (V) | 12.98[1] |
| Characteristics | |
| Type | SAB(rs)c[1] |
| Size | ~56,800 ly (17.41 kpc) (estimated)[1] |
| Apparent size (V) | 1.6′ × 1.5′[1] |
| Other designations | |
| IRAS 11013+2818, 2MASX J11040298+2802125, UGC 6128, MCG +05-26-041, PGC 33432, CGCG 155-051[1] | |
NGC 3512 is an intermediate spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 1,677±21 km/s, which corresponds to a Hubble distance of 80.7 ± 5.7 Mly (24.73 ± 1.76 Mpc).[1] However, four non-redshift measurements give a farther mean distance of 113.50 ± 11.20 Mly (34.800 ± 3.434 Mpc).[2] It was discovered by German-British astronomer William Herschel on 11 April 1785.[3][4]
NGC 3512 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.[1]
NGC 3504 group
[edit]NGC 3512 is a member of the NGC 3504 Group (also known as LGG 227), which is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the western edge of the Virgo Supercluster.[5] There are eight other galaxies in the group, including NGC 3380, NGC 3400, NGC 3414, NGC 3451, NGC 3504, UGC 5921 and UGC 5958.[6][7] This NGC 3504 group is also mentioned by Abraham Mahtessian in his research paper published in 1998.[8]
Supernova
[edit]One supernova has been observed in NGC 3512:
- SN 2001fv (Type II, mag. 16.4) was discovered by British amateur astronomer Mark Armstrong on 3 November 2001.[9][10]
See also
[edit]References
[edit]- 1 2 3 4 5 6 7 8 9 10 11 "Results for object NGC 3512". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 25 June 2026.
- 1 2 "Distance Results for NGC 3512". NASA/IPAC Extragalactic Database. NASA. Retrieved 25 June 2026.
- ↑ Herschel, William (1786). "Catalogue of One Thousand New Nebulae and Clusters of Stars" (PDF). Philosophical Transactions of the Royal Society of London. 76: 457–499. Bibcode:1786RSPT...76..457H. doi:10.1098/rstl.1786.0027.
- ↑ Seligman, Courtney. "New General Catalogue Objects: NGC 3512". Celestial Atlas. Retrieved 25 June 2026.
- ↑ "The Leo III Groups". Atlas of the Universe. Retrieved 25 June 2026.
- ↑ Garcia, A. M. (1 July 1993). "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.
- ↑ "LGG 227". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 19 June 2026.
- ↑ Mahtessian, A. P. (1 July 1998). "Groups of galaxies. III. Some empirical characteristics". Astrophysics. 41 (3): 308–321. Bibcode:1998Ap.....41..308M. doi:10.1007/BF03036100. ISSN 0571-7256.
- ↑ Hurst, G. M.; Armstrong, M. (2001). "Supernova 2001fv in NGC 3512". International Astronomical Union Circular (7750): 1. Bibcode:2001IAUC.7750....1H.
- ↑ "SN 2001fv". Transient Name Server. IAU. Retrieved 25 June 2026.
External links
[edit]
Media related to NGC 3512 at Wikimedia Commons- NGC 3512 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
| Morphology | |
|---|---|
| Structure | |
| Active nuclei | |
| Energetic galaxies | |
| Low activity | |
| Interaction | |
| Lists | |
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