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.[1][2]
It was discovered by French astronomer, Stephane Javelle on November 25, 1897[3] 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.[4]
IC 5337 is a jellyfish galaxy, mainly due to ram pressure.[5][6][7] 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.[5] It has a stellar mass of 3.2 × 1011 M⊙[8] and contains an active galactic nucleus likely trigged by accretion of matter into its supermassive black hole.[9]
In addition, IC 5337 also shows an X-ray source.[10]
See also
[edit]References
[edit]- ^ "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.
- ^ a b 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.
