NGC 5032
| NGC 5032 | |
|---|---|
 The barred spiral galaxy NGC 5032. | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 13h 13m 26.9488s[1] |
| Declination | +27° 48′ 08.56″[1] |
| Redshift | 0.021398[1] |
| Heliocentric radial velocity | 6415 ± 1 km/s[1] |
| Distance | 321.1 ± 22.5 Mly (98.45 ± 6.90 Mpc)[1] |
| Apparent magnitude (V) | 12.8[1] |
| Characteristics | |
| Type | SB(r)b[1] |
| Size | ~223,900 ly (68.64 kpc) (estimated)[1] |
| Apparent size (V) | 2.1' x 1.1'[1] |
| Other designations | |
| IRAS F00009-1101, 2MASX J13132694+2748086, UGC 8300, MCG +05-31-160, PGC 45947, CGCG 160-166[1] | |
NGC 5032 is a barred spiral galaxy in the constellation of Coma Berenices. Its velocity with respect to the cosmic microwave background is 6675 ± 18 km/s, which corresponds to a Hubble distance of 98.45 ± 6.90 Mpc (∼321 million light-years).[1] It was discovered by German-British astronomer William Herschel on 11 April 1785.[2]
NGC 5032 was used by Gérard de Vaucouleurs as a galaxy of morphological type (R′)SAB(rs)b in his atlas of galaxies.[2]
NGC 5032 is classified as a LINER galaxy, i.e. it has a type of nucleus that is defined by its spectral line emission which has weakly ionized or neutral atoms, while the spectral line emission from strongly ionized atoms is relatively weak.[1]
NGC 5032 forms a interacting galaxy pair with PGC 45940 (sometimes called NGC 5032B).[2] Erik Holmberg included the group in his catalog of double and multiple galaxies, with the designation Holm 513.[3] NGC 5032 is also on the outskirts of the Coma Cluster, identified as ComaFC 370.[4]
Two supernovae have been observed in NGC 5032: SN 2016iuc (type Ia, mag 16.7)[5] and SN 2024rkc (type Ia, mag. 18.7).[6]
See also
[edit]References
[edit]- ^ a b c d e f g h i j k l "NASA/IPAC Extragalactic Database". Results for NGC 5032. Retrieved 5 August 2024.
- ^ a b c Seligman, Courtney. "Celestial Atlas Entry for NGC 5032". cseligman.com. Retrieved 8 August 2024.
- ^ Holmberg, Erik (1937). "A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems". Annals of the Observatory of Lund. 6: 1. Bibcode:1937AnLun...6....1H.
- ^ Fuller, C.; Davies, J. I.; Smith, M. W. L.; Valiante, E.; Eales, S.; Bourne, N.; Dunne, L.; Dye, S.; Furlanetto, C.; Ibar, E.; Ivison, R.; Maddox, S.; Sansom, A.; Michałowski, M. J.; Davis, T. (2016). "H-ATLAS: The far-infrared properties of galaxies in and around the Coma cluster". Monthly Notices of the Royal Astronomical Society. 458 (1): 582. arXiv:1603.02970. Bibcode:2016MNRAS.458..582F. doi:10.1093/mnras/stw305.
- ^ "Transient Name Server". Entry for SN 2016iuc. Retrieved 9 August 2024.
- ^ "Transient Name Server". Entry for SN 2024rkc. Retrieved 9 August 2024.
External links
[edit]
Media related to NGC 5032 at Wikimedia Commons- NGC 5032 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
