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| NGC 5665 | |
|---|---|
 Hubble Space Telescope view of NGC 5665 | |
| Observation data (J2000 epoch) | |
| Constellation | Boötes |
| Right ascension | 14h 32m 25.796s[1] |
| Declination | +08° 04′ 42.43″[1] |
| Redshift | 0.007431±0.000017[2] |
| Heliocentric radial velocity | 2,237 km/s[3] |
| Distance | 53.6 ± 7.7 Mly (16.44 ± 2.37 Mpc)[3] |
| Apparent magnitude (V) | 12.7[4] |
| Apparent magnitude (B) | 12.50[5] |
| Characteristics | |
| Type | SAB(rs)c pec?[6] |
| Mass | 6×1010[5] M☉ |
| Apparent size (V) | 1.653′ × 1.257′[1] |
| Other designations | |
| GC 3923, IRAS F14299+0818, 2MASX J14322579+0804424, NGC 5665, UGC 9352, LEDA 51953, MCG +01-37-024, PGC 51953, CGCG 047.084, VV 412[7] | |
NGC 5665 is a spiral galaxy in the northern constellation of Boötes. It was discovered on January 30, 1784 by German-British astronomer William Herschel.[8] This galaxy is located at a distance of 53.6 ± 7.7 million light-years (16.44 ± 2.37 Mpc),[3] and is receding with a heliocentric radial velocity of 2,237 km/s.[3] It is cataloged in Halton Arp's Atlas of Peculiar Galaxies as object number 49.[5]
The morphological classification of NGC 5665 is unclear and differs by author.[5] In the De Vaucouleurs system it was classified as SAB(rs)c pec?,[6] which indicates a weakly-barred spiral galaxy (SAB) with a transitional inner ring structure (rs), loosely wound spiral arms (c), and suspected peculiarities (pec?). The galactic plane is inclined at an angle of 53°±5° to the plane of the sky,[3] with the major axis aligned along a position angle of 145°.[5]
Evidence suggests that NGC 5665 underwent a gravitational interaction with another galaxy some 500 million years ago, swallowing a smaller companion.[5] It is somewhat asymmetrical in appearance,[6] retaining a single main spiral arm and the remains of several others. The galaxy is rich in dust and gas with a small bar at the center. There are numerous sites of star formation in the arm that match the age of the interaction.[5] The spectrum of the core is a blend between a LINER and an H II region.[6]
References
[edit]- ^ a b c Skrutskie, Michael F.; et al. (February 1, 2006), "The Two Micron All Sky Survey (2MASS)", The Astronomical Journal, 131 (2): 1163–1183, Bibcode:2006AJ....131.1163S, doi:10.1086/498708, ISSN 0004-6256, S2CID 18913331.
- ^ Chengalur, Jayaram N.; Salpeter, E. E.; Terzian, Yervant (December 1993), "Dynamics of Binary Galaxies. I. Wide Pairs", Astrophysical Journal, 419: 30, Bibcode:1993ApJ...419...30C, doi:10.1086/173456.
- ^ a b c d e Kourkchi, Ehsan; et al. (October 23, 2020), "Cosmicflows-4: The Catalog of ∼10,000 Tully–Fisher Distances", The Astrophysical Journal, 902 (2): 145, arXiv:2009.00733, Bibcode:2020ApJ...902..145K, doi:10.3847/1538-4357/abb66b, ISSN 1538-4357.
- ^ "NED results for object NGC 5665", NASA/IPAC Extragalactic Database, NASA, retrieved 2015-10-19.
- ^ a b c d e f g Artamonov, B. P.; et al. (September 2000), "BVRI CCD photometry of the peculiar galaxies NGC 5605 and NGC 5665", Astronomy Reports, 44 (9): 569–578, Bibcode:2000ARep...44..569A, doi:10.1134/1.1307552.
- ^ a b c d Thomas, H. C.; Dunne, L.; Clemens, M. S.; Alexander, P.; Eales, S.; Green, D. A. (February 2002), "The distribution of atomic gas and dust in nearby galaxies - I. Presentation of matched-resolution VLA H I and SCUBA 850-μm maps", Monthly Notices of the Royal Astronomical Society, 329 (4): 747–758, Bibcode:2002MNRAS.329..747T, doi:10.1046/j.1365-8711.2002.05035.x.
- ^ "NGC 5665", SIMBAD, Centre de données astronomiques de Strasbourg, retrieved 2024-04-14.
- ^ Seligman, COurtney, "NGC Objects: NGC 5650 - 5699", Celestial Atlas, retrieved 2024-04-14.
External links
[edit]
Media related to NGC 5665 at Wikimedia Commons- Image NGC 5665
- Distance Archived 2011-06-07 at the Wayback Machine
- SIMBAD Data
