| NGC 5735 | |
|---|---|
| 👁 Image NGC 5735 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Boötes |
| Right ascension | 14h 42m 33.2479s[1] |
| Declination | +28° 43′ 35.420″[1] |
| Redshift | 0.012408±0.00000700[1] |
| Heliocentric radial velocity | 3,720±2 km/s[1] |
| Distance | 190.48 ± 2.45 Mly (58.400 ± 0.751 Mpc)[2] |
| Group or cluster | NGC 5653 Group (LGG 383) |
| Apparent magnitude (V) | 13.10[1] |
| Characteristics | |
| Type | SB(rs)bc[1] |
| Size | ~155,200 ly (47.57 kpc) (estimated)[1] |
| Apparent size (V) | 2.4′ × 1.9′[1] |
| Other designations | |
| IRAS 14403+2856, 2MASX J14423324+2843347, UGC 9481, MCG +05-35-007, PGC 52535, CGCG 164-013[1] | |
NGC 5735 is a barred spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 3,894±12 km/s, which corresponds to a Hubble distance of 187.3 ± 13.1 Mly (57.44 ± 4.02 Mpc).[1] Additionally, three non-redshift measurements give a similar mean distance of 190.48 ± 2.45 Mly (58.400 ± 0.751 Mpc).[2] It was discovered by German-British astronomer William Herschel on 17 May 1784.[3][4]
NGC 5735 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.[5][6]
NGC 5653 group
[edit]NGC 5735 is a member of the NGC 5653 group (also known as LGG 383). This group contains 15 galaxies, including NGC 5629, NGC 5635 [fr], NGC 5639 [fr], NGC 5641, NGC 5642, NGC 5653, NGC 5659 [fr], NGC 5657 [fr], NGC 5672 [fr], NGC 5703 [fr], IC 4397, UGC 9253 [d], UGC 9268 [d], and UGC 9302 [d].[7][8]
Supernova
[edit]One supernova has been observed in NGC 5735:
- SN 2006qp (TypeIIb, mag. 17.1) was discovered by Kōichi Itagaki on 25 November 2006.[9][10]
See also
[edit]References
[edit]- ^ a b c d e f g h i j "Results for object NGC 5735". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 24 March 2026.
- ^ a b "Distance Results for NGC 5735". NASA/IPAC Extragalactic Database. NASA. Retrieved 24 March 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 5735". Celestial Atlas. Retrieved 24 March 2026.
- ^ Toba, Y.; Oyabu, S.; Matsuhara, H.; Malkan, M. A.; Gandhi, P.; Nakagawa, T.; Isobe, N.; Shirahata, M.; Oi, N.; Ohyama, Y.; Takita, S.; Yamauchi, C.; Yano, K. (2014). "Luminosity and Redshift Dependence of the Covering Factor of Active Galactic Nuclei viewed with WISE and Sloan Digital Sky Survey". The Astrophysical Journal. 788 (1): 45. arXiv:1404.4937. Bibcode:2014ApJ...788...45T. doi:10.1088/0004-637X/788/1/45.
- ^ "NGC 5735". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 24 March 2026.
- ^ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.
- ^ "LGG 383". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 24 March 2026.
- ^ Nakano, S.; Naito, H.; Shimada, M.; Takaki, T.; Yamaoka, H. (2006). "Supernova 2006qp in NGC 5735". Central Bureau Electronic Telegrams (764): 1. Bibcode:2006CBET..764....1N.
- ^ "SN 2006qp". Transient Name Server. IAU. Retrieved 24 March 2026.
External links
[edit]- 👁 Wikimedia Commons logo
Media related to NGC 5735 at Wikimedia Commons - NGC 5735 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
