NGC 5917
(Redirected from Arp 254)
| NGC 5917 | |
|---|---|
 NGC 5917 imaged by the Hubble Space Telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Libra[1] |
| Right ascension | 15h 21m 32.550s[2] |
| Declination | −07° 22′ 37.52″[2] |
| Redshift | 0.00635[3] |
| Heliocentric radial velocity | 1,934.1[4] |
| Distance | 90.4 ± 6.2 Mly (27.73 ± 1.90 Mpc)[3] |
| Apparent magnitude (V) | 14.5[5] |
| Apparent magnitude (B) | 13.7[3] |
| Characteristics | |
| Type | Sb pec:[5] |
| Apparent size (V) | 1.60′ × 0.9′[6] |
| Notable features | Interacting galaxy |
| Other designations | |
| GSC 05014-00224, IRAS F15188-0711, 2MASX J15213256-0722376, NGC 5917, LEDA 54809, MCG -01-39-002, PGC 54809[7] | |
NGC 5917 is a spiral galaxy located in the constellation of Libra. It was discovered by English astronomer John Herschel on 16 July 1835.[8] This galaxy is located at a distance of 90.4 ± 6.2 million light-years (27.73 ± 1.90 Mpc) from the Milky Way,[3] and is receding with a heliocentric radial velocity of 1,934.1 km/s.[4] It is interacting with the neighboring galaxy, PGC 54817, at an angular separation of 4.2′. Tidal tails extend from PGC 54817 to the halo of NGC 5917.[5]
One supernova has been observed in NGC 5917. SN 1990Q (type II, mag. 18) was discovered by Christian Pollas on 24 June 1990.[9][10][11]
References
[edit]- ^ "A cosmic conversation". www.spacetelescope.org. Retrieved 2 May 2017.
- ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ a b c d Cai, Y.-Z; et al. (October 2021). "Intermediate-luminosity red transients: Spectrophotometric properties and connection to electron-capture supernova explosions". Astronomy and Astrophysics. 654. A157. arXiv:2108.05087. Bibcode:2021A&A...654A.157C. doi:10.1051/0004-6361/202141078.
- ^ a b Meyer, M. J.; et al. (June 2004). "The HIPASS catalogue - I. Data presentation". Monthly Notices of the Royal Astronomical Society. 350 (4): 1195–1209. arXiv:astro-ph/0406384. Bibcode:2004MNRAS.350.1195M. doi:10.1111/j.1365-2966.2004.07710.x. S2CID 10336076.
- ^ a b c König, Michael; Binnewies, Stefan (2017). The Cambridge Photographic Atlas of Galaxies. Cambridge University Press. p. 295. ISBN 9781107189485.
- ^ "Revised NGC Data for NGC 5640". spider.seds.org. Retrieved December 8, 2017.
- ^ "NGC 5917". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2 May 2017.
- ^ Seligman, COurtney. "New General Catalog Objects: NGC 5900 - 5949". cseligman.com. Retrieved 2017-12-08.
- ^ Pollas, C.; Albanese, D.; Turatto, M.; Cappellaro, E.; Benetti, S. (1990). "Supernova 1990Q in NGC 5917". International Astronomical Union Circular (5040): 1. Bibcode:1990IAUC.5040....1P.
- ^ "SN 1990Q". Transient Name Server. IAU Supernova Working Group. June 24, 1990. Retrieved 2024-05-20.
- ^ Benetti, S.; et al. (June 1990). Green, D. W. E. (ed.). "Supernova 1990Q in NGC 5917". IAU Circular. 5042: 1. Bibcode:1990IAUC.5042....1B.
External links
[edit]
Media related to NGC 5917 at Wikimedia Commons- NGC 5917 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
 | This spiral galaxy article is a stub. You can help Wikipedia by expanding it. |