NGC 5719
| NGC 5719 | |
|---|---|
 The intermediate spiral galaxy NGC 5719. | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 14h 40m 56.37s |
| Declination | −00° 19′ 05.78″ |
| Redshift | 0.005781 |
| Heliocentric radial velocity | 1,733 km/s |
| Distance | 94.2 Mly (28.89 Mpc) |
| Apparent magnitude (V) | 0.13 |
| Apparent magnitude (B) | 0.17 |
| Characteristics | |
| Type | SAB(s)ab pec |
| Size | 26.68 kiloparsecs (87,000 light-years) (diameter; 2MASS K-band total isophote) [1] |
| Other designations | |
| NGC 5658, UGC 9462, PGC 52455, IRAS 14383-0006, MCG +00-37-024, CGCG 019-079 | |
NGC 5719 is an intermediate or barred spiral galaxy located in the constellation Virgo. It is located at a distance of 94 million light years from Earth.[1] It was first discovered by William Herschel in April 1787, but also observed by John Herschel in April 1828 and by George Phillips Bond in March 1853, who catalogued the object as NGC 5658 under the New General Catalogue.[2]
The luminosity class of NGC 5719 is I-II and it has a broad HI line. Additionally, it is a narrow line active galaxy (NLAGN).[1] In far infrared (40-400 ɥm), the luminosity of NGC 5719 is 1.70 x 1010 Lʘ (1010.23 Lʘ) while its total luminosity in infrared (from the 8-1000 ɥm range) is 2.24 x 10 Lʘ (1010.35 Lʘ).[3]
Characteristics
[edit]NGC 5719 is classified as an Sab galaxy found almost edge-on. It is interacting with a nearby face-on Sbc companion, NGC 5713.[4][5] The dust lane of the galaxy is tilted, as well as bent significantly and inclined to its major axis.[6]
The galaxy has two HI tidal bridges which loop around it and are connecting with NGC 5713. There is a detection of two HI tidal tails leaving NGC 5713. Inside the disk of the galaxy (NGC 5719), ionized and neutral hydrogen are present. Both are counter-rotating in respect to the main stellar disk.[4][7] When measuring the kinematics of both counter-rotating stellar disks and the ionized-gas disk, they extend by about 40 arcsec (4.3 kpc) from NGC 5719's center.[7]
NGC 5746 group
[edit]
NGC 5719 is part of the NGC 5746 group according to A.M. Garcia. In this galaxy group there are 31 members including NGC 5636, NGC 5638, NGC 5668, NGC 5690, NGC 5691, NGC 5692, NGC 5701, NGC 5705, NGC 5713, NGC 5725, NGC 5740, NGC 5746, NGC 5750, IC 1022, IC 1024 and IC 1048.[8] Together the NGC 5719 group is part of the Virgo III cluster, one of the clusters in the Virgo Supercluster.[9]
References
[edit]- ^ a b c "By Name NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2024-10-09.
- ^ "New General Catalog Objects: NGC 5700 - 5749". cseligman.com. Retrieved 2024-10-09.
- ^ Sanders, D.B.; Mazzarella, J.M.; Kim, D.-C.; Surace, J.A.; Soifer, B.T. (August 2003). "The IRAS Revised Bright Galaxy Sample (RBGS)". The Astronomical Journal. 126 (4): 1607–1664. arXiv:astro-ph/0306263. doi:10.1086/376841.
- ^ a b Vergani, D.; Pizzella, A.; Corsini, E. M.; van Driel, W.; Buson, L. M.; Dettmar, R. -J.; Bertola, F. (2007-03-01). "NGC 5719/13: interacting spirals forming a counter-rotating stellar disc". Astronomy and Astrophysics. 463 (3): 883–892. arXiv:astro-ph/0611426. Bibcode:2007A&A...463..883V. doi:10.1051/0004-6361:20066413. ISSN 0004-6361.
- ^ de Vaucouleurs, Gerard Henri; de Vaucouleurs, Antoinette; Shapley, Harlow (1964-01-01). Reference catalogue of bright galaxies. Bibcode:1964rcbg.book.....D.
- ^ Luttickle, R.; Pohlen, M.; Dettmar, R.J. (2004). "Box- and peanut-shaped bulges III. A new class of bulges: Thick Boxy Bulges" (PDF). Astronomy & Astrophysics. 417: 527–539. arXiv:astro-ph/0401057. Bibcode:2004A&A...417..527L. doi:10.1051/0004-6361:20031782.
- ^ a b Coccato, L.; Morelli, L.; Corsini, E. M.; Buson, L.; Pizzella, A.; Vergani, D.; Bertola, F. (2011-03-01). "Dating the formation of the counter-rotating stellar disc in the spiral galaxy NGC 5719 by disentangling its stellar populations". Monthly Notices of the Royal Astronomical Society: Letters. 412 (1): L113–L117. arXiv:1101.3092. Bibcode:2011MNRAS.412L.113C. doi:10.1111/j.1745-3933.2011.01016.x. ISSN 1745-3933.
- ^ Garcia, A. M. (1993-07-01). "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.
- ^ "The Virgo III Groups". www.atlasoftheuniverse.com. Retrieved 2024-10-09.
