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PGC 2456

From Wikipedia, the free encyclopedia
Galaxy in the constellation Cetus
PGC 2456
Hubble Space Telescope of PGC 2456 and its surrounding galaxiesPGC 2800504 and2MASX J00413329-0914569
Observation data (J2000epoch)
ConstellationCetus
Right ascension00h 41m 30.29s
Declination-09d 15m 45.85s
Redshift0.044674
Distance617Mly (189.17Mpc)
Group orclusterAbell 85
Apparent magnitude (V)0.10
Apparent magnitude (B)0.13
Characteristics
TypecD, Sy
Other designations
PGC 2456,PGC 93189,NVSS J004130-091545, KAZ 364, WINGS J004130.29-091546.0, NSA 127503, 2CXO J001430.3-091546, JO201

PGC 2456 known asKAZ 364 andJO201, is aspiral galaxy located in the constellation ofCetus. It is located 617 millionlight-years away from theSolar System.[1] A member of Abell 85, PGC 2456 lies 360 kiloparsecs from the brightest cluster galaxy,Holmberg 15A.[2]

PGC 2456 contains anactive galactic nucleus.[3] It is a low-excitationradio galaxy,[4] with a stellar mass of 3.6 x 1010M.[5]

PGC 2456 is considered ajellyfish galaxy due to the fact the tendrils are seen drifting downwards from its core.[6][7] It exhibits intensivestar formation in its tendrils and is the Ultraviolet-brightest cluster galaxy in Abell 85.[8][9]

Such jellyfish galaxies are formed when galaxies like PGC 2456, moves through high speeds across thegalaxy clusters, causing ram pressure to strip gas. According to studies, researchers estimated PGC 2456 might have lost about 50% of its mass when undergoingram-pressure stripping.[10]

See also

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References

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  1. ^"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2024-04-20.
  2. ^Ramatsoku, M.; Serra, P.; Poggianti, B. M.; Moretti, A.; Gullieuszik, M.; Bettoni, D.; Deb, T.; Franchetto, A.; Gorkom, J. H. van; Jaffé, Y.; Tonnesen, S.; Verheijen, M. a. W.; Vulcani, B.; Andati, L. a. L.; Blok, E. de (2020-08-01)."GASP - XXVI. HI gas in jellyfish galaxies: The case of JO201 and JO206".Astronomy & Astrophysics.640: A22.arXiv:2006.11543.Bibcode:2020A&A...640A..22R.doi:10.1051/0004-6361/202037759.ISSN 0004-6361.
  3. ^Radovich, Mario; Poggianti, Bianca; Jaffé, Yara L; Moretti, Alessia; Bettoni, Daniela; Gullieuszik, Marco; Vulcani, Benedetta; Fritz, Jacopo (2019-03-19)."GASP – XIX. AGN and their outflows at the centre of jellyfish galaxies".Monthly Notices of the Royal Astronomical Society.486 (1):486–503.arXiv:1905.08972.doi:10.1093/mnras/stz809.ISSN 0035-8711.
  4. ^Lin, Yen-Ting; Huang, Hung-Jin; Chen, Yen-Chi (2018-05-01)."An Analysis Framework for Understanding the Origin of Nuclear Activity in Low-power Radio Galaxies".The Astronomical Journal.155 (5): 188.arXiv:1803.02482.Bibcode:2018AJ....155..188L.doi:10.3847/1538-3881/aab5b4.ISSN 0004-6256.
  5. ^Vulcani, Benedetta; Poggianti, Bianca M.; Gullieuszik, Marco; Moretti, Alessia; Tonnesen, Stephanie; Jaffé, Yara L.; Fritz, Jacopo; Fasano, Giovanni; Bettoni, Daniela (2018-10-17)."Enhanced Star Formation in Both Disks and Ram-pressure-stripped Tails of GASP Jellyfish Galaxies".The Astrophysical Journal Letters.866 (2): L25.arXiv:1810.05164.Bibcode:2018ApJ...866L..25V.doi:10.3847/2041-8213/aae68b.ISSN 2041-8205.
  6. ^information@eso.org."Galactic Seascape".www.spacetelescope.org. Retrieved2024-04-20.
  7. ^Anderson, Natali (2023-02-27)."Hubble Finds Star-Forming Clumps in Six Jellyfish Galaxies | Sci.News".Sci.News: Breaking Science News. Retrieved2024-07-26.
  8. ^George, K.; Poggianti, B. M.; Gullieuszik, M.; Fasano, G.; Bellhouse, C.; Postma, J.; Moretti, A.; Jaffé, Y.; Vulcani, B.; Bettoni, D.; Fritz, J.; Côté, P.; Ghosh, S. K.; Hutchings, J. B.; Mohan, R. (2018-09-01)."UVIT view of ram-pressure stripping in action: star formation in the stripped gas of the GASP jellyfish galaxy JO201 in Abell 85".Monthly Notices of the Royal Astronomical Society.479 (3):4126–4135.arXiv:1803.06193.Bibcode:2018MNRAS.479.4126G.doi:10.1093/mnras/sty1452.ISSN 0035-8711.
  9. ^George, Koshy; Poggianti, B. M.; Gullieuszik, M.; Fasano, G.; Bellhouse, C.; Postma, J.; Moretti, A.; Jaffé, Y.; Vulcani, B.; Bettoni, D.; Fritz, J.; Côté, P.; Ghosh, S. K.; Hutchings, J. B.; Mohan, R. (2018-09-21)."Ultra-Violet Imaging Telescope view of ram-pressure stripping in action: Star formation in the stripped gas of the GASP jellyfish galaxy JO201 in Abell 85".Monthly Notices of the Royal Astronomical Society.479 (3):4126–4135.arXiv:1803.06193.Bibcode:2018MNRAS.479.4126G.doi:10.1093/mnras/sty1452.ISSN 0035-8711.
  10. ^Bellhouse, C.; Jaffé, Y. L.; Hau, G. K. T.; McGee, S. L.; Poggianti, B. M.; Moretti, A.; Gullieuszik, M.; Bettoni, D.; Fasano, G.; D'Onofrio, M.; Fritz, J.; Omizzolo, A.; Sheen, Y. -K.; Vulcani, B. (2017-07-01)."GASP. II. A MUSE View of Extreme Ram-Pressure Stripping along the Line of Sight: Kinematics of the Jellyfish Galaxy JO201".The Astrophysical Journal.844 (1): 49.arXiv:1704.05087.Bibcode:2017ApJ...844...49B.doi:10.3847/1538-4357/aa7875.ISSN 0004-637X.
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