IC 5337
| IC 5337 | |
|---|---|
 Hubble Space Telescope image of IC 5337 (lower right) and IC 5338 (upper left) | |
| Observation data (J2000 epoch) | |
| Constellation | Pegasus |
| Right ascension | 23hh 36m 25.03s |
| Declination | +21° 09′ 01.98″ |
| Redshift | 0.054988 |
| Heliocentric radial velocity | 16,485 km/s |
| Distance | 800 Mly (245.2 Mpc) |
| Group or cluster | Abell 2626 |
| Apparent magnitude (V) | 0.17 |
| Apparent magnitude (B) | 0.23 |
| Characteristics | |
| Type | S0, S? |
| Size | 175,000 ly (estimated) |
| Apparent size (V) | 0.8' x 0.1' |
| Other designations | |
| PGC 71875, MCG +03-60-012, AGC 330572, 2MASX J23362506+2109028, LEDA 71875, Z455-25, JW100 | |
IC 5337 or JW100, is a spiral galaxy located 800 million light-years away from the Solar System in the constellation of Pegasus.
It was discovered by French astronomer, Stephane Javelle on November 25, 1897 and is probably gravitationally bound to IC 5338, the brightest cluster galaxy in Abell 2626. According to SIMBAD, IC 5337 is considered an emission-line galaxy.
IC 5337 is a jellyfish galaxy, mainly due to ram pressure. Star-forming gas are thrown about, as the galaxy penetrates through the thin gas layer and causing them to drip from the galaxy's disc, giving it its unique appearance of a cosmic jellyfish. It has a stellar mass of 3.2 × 1011 M☉ and contains an active galactic nucleus likely trigged by accretion of matter into its supermassive black hole.
In addition, IC 5337 also shows an X-ray source.
See also
References
- ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-20.
- ↑ "IC 5337 - Spiral Galaxy in Pegasus | TheSkyLive.com". theskylive.com. Retrieved 2024-04-20.
- ↑ "Index Catalog Objects: IC 5300 - 5349". cseligman.com. Retrieved 2024-04-20.
- ↑ "IC 5337". simbad.u-strasbg.fr. Retrieved 2024-04-20.
- 1 2 information@eso.org. "Portrait of a galactic jellyfish". www.spacetelescope.org. Retrieved 2024-04-20.
- ↑ information@eso.org. "Example of a jellyfish galaxy". www.eso.org. Retrieved 2024-04-20.
- ↑ Poggianti, B. M.; Fasano, G.; Omizzolo, A.; Gullieuszik, M.; Bettoni, D.; Moretti, A.; Paccagnella, A.; Jaffé, Y. L.; Vulcani, B.; Fritz, J.; Couch, W.; D'Onofrio, M. (2016-03-01). "Jellyfish Galaxy Candidates at Low Redshift". The Astronomical Journal. 151 (3): 78. arXiv:1504.07105. Bibcode:2016AJ....151...78P. doi:10.3847/0004-6256/151/3/78. ISSN 0004-6256.
- ↑ Poggianti, Bianca M.; Ignesti, Alessandro; Gitti, Myriam; Wolter, Anna; Brighenti, Fabrizio; Biviano, Andrea; George, Koshy; Vulcani, Benedetta; Gullieuszik, Marco; Moretti, Alessia; Paladino, Rosita; Bettoni, Daniela; Franchetto, Andrea; Jaffé, Yara L.; Radovich, Mario (2019-12-01). "GASP XXIII: A Jellyfish Galaxy as an Astrophysical Laboratory of the Baryonic Cycle". The Astrophysical Journal. 887 (2): 155. arXiv:1910.11622. Bibcode:2019ApJ...887..155P. doi:10.3847/1538-4357/ab5224. ISSN 0004-637X.
- ↑ Poggianti, Bianca M.; Jaffé, Yara L.; Moretti, Alessia; Gullieuszik, Marco; Radovich, Mario; Tonnesen, Stephanie; Fritz, Jacopo; Bettoni, Daniela; Vulcani, Benedetta; Fasano, Giovanni; Bellhouse, Callum; Hau, George; Omizzolo, Alessandro (2017-08-01). "Ram-pressure feeding of supermassive black holes". Nature. 548 (7667): 304–309. arXiv:1708.09036. Bibcode:2017Natur.548..304P. doi:10.1038/nature23462. ISSN 0028-0836. PMID 28816245.
- ↑ Wong, Ka-Wah; Sarazin, Craig L.; Blanton, Elizabeth L.; Reiprich, Thomas H. (2008-07-01). "XMM-Newton and Chandra Observations of Abell 2626: Interacting Radio Jets and Cooling Core with Jet Precession?". The Astrophysical Journal. 682 (1): 155–174. arXiv:0803.1680. Bibcode:2008ApJ...682..155W. doi:10.1086/588272. ISSN 0004-637X.
