PGC 29820

Last updated
PGC 29820
PGC29820 Potw2315a.jpg
PGC 29820 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
Constellation Sextans
Right ascension 10h 13m 46.82s
Declination -00d 54m 51.0s
Redshift 0.04244
Heliocentric radial velocity 12,723 km/s
Distance 600 Mly (183.96 Mpc)
Group or cluster Abell 957
Apparent magnitude  (V)0.11
Apparent magnitude  (B)0.15
Characteristics
Type Sb(f), Seyfert 2
Size120,000 ly
Other designations
LEDA 29820, CGCG 008-077, 2dFGRS N288Z210, AGC 500048, NVSS J101346-005449, JO204

PGC 29820 (known as JO204) is a spiral galaxy 600 million light-years from the Solar System, in the Sextans constellation. [1] The galaxy is about 120,000 light-years in diameter and is a member of Abell 957, a low-mass galaxy cluster. [2] The first known reference to this galaxy is from volume I of the Catalogue of Galaxies and of Clusters of Galaxies compiled by Fritz Zwicky in 1961, where it was listed as CGCG 008-077. [3]

Contents

Characteristics

PGC 29820 is classified a massive galaxy with a stellar mass of M* = 4 x1010 M. [4] It contains an active galactic nucleus with double-peaked narrow lines. [5] [6] Moreover, it is also a Seyfert 2 galaxy. [7]

PGC 29820 is classified a jellyfish galaxy. [8] [9] [10] According to Gullieuszik, the galaxy is currently in a first phrase of infalling into the cluster where it is subjected to ram pressure by the intracluster medium. [2]

Because dense gas is compressed, it eventually collapses to form new stars in both the galaxy's tail and its disk. [4] According to researchers, the stars inside the tail, has a star formation rate of 0.22 M○ yr1 [11] which began during the last 500 million years. [2]

In additional, PGC 29820 shows a large presence of molecular gas making up H2 mass of 8.3 x 109 M○. Looking at ratio of total molecular hydrogen mass and stellar mass, it is estimated as 0.42. [12]

See also

References

  1. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 18 April 2024.
  2. 1 2 3 Gullieuszik, Marco; Poggianti, Bianca M.; Moretti, Alessia; Fritz, Jacopo; Jaffé, Yara L.; Hau, George; Bischko, Jan C.; Bellhouse, Callum; Bettoni, Daniela; Fasano, Giovanni; Vulcani, Benedetta; D'Onofrio, Mauro; Biviano, Andrea (1 September 2017). "GASP. IV. A Muse View of Extreme Ram-pressure-stripping in the Plane of the Sky: The Case of Jellyfish Galaxy JO204". The Astrophysical Journal. 846 (1): 27. arXiv: 1708.09035 . Bibcode:2017ApJ...846...27G. doi: 10.3847/1538-4357/aa8322 . ISSN   0004-637X.
  3. ↑ Zwicky, F.; Herzog, E.; Wild, P. (1961). Catalogue of galaxies and of clusters of galaxies, Vol. I. p. 26. Bibcode:1961cgcg.book.....Z. Archived from the original on 19 August 2023.
  4. 1 2 Deb, Tirna; Verheijen, Marc A W; Gullieuszik, Marco; Poggianti, Bianca M; van Gorkom, Jacqueline H; Ramatsoku, Mpati; Serra, Paolo; Moretti, Alessia; Vulcani, Benedetta; Bettoni, Daniela; Jaffé, L Yara; Tonnesen, Stephanie; Fritz, Jacopo (23 April 2020). "GASP XXV: neutral hydrogen gas in the striking jellyfish galaxy JO204". Monthly Notices of the Royal Astronomical Society. 494 (4): 5029–5043. arXiv: 2004.04754 . doi: 10.1093/mnras/staa968 . ISSN   0035-8711.
  5. ↑ Wang, Jian-Min; Chen, Yan-Mei; Hu, Chen; Mao, Wei-Ming; Zhang, Shu; Bian, Wei-Hao (1 November 2009). "Active Galactic Nuclei with Double-Peaked Narrow Lines: Are they Dual Active Galactic Nuclei?". The Astrophysical Journal. 705 (1): L76 –L80. arXiv: 0910.0580 . Bibcode:2009ApJ...705L..76W. doi:10.1088/0004-637X/705/1/L76. ISSN   0004-637X.
  6. ↑ Nevin, R.; Comerford, J.; Müller-Sánchez, F.; Barrows, R.; Cooper, M. (1 November 2016). "The Origin of Double-peaked Narrow Lines in Active Galactic Nuclei. II. Kinematic Classifications for the Population at z < 0.1". The Astrophysical Journal. 832 (1): 67. arXiv: 1609.04018 . Bibcode:2016ApJ...832...67N. doi: 10.3847/0004-637X/832/1/67 . ISSN   0004-637X.
  7. ↑ Véron-Cetty, M. -P.; Véron, P. (1 August 2006). "A catalogue of quasars and active nuclei: 12th edition". Astronomy and Astrophysics. 455 (2): 773–777. Bibcode:2006A&A...455..773V. doi:10.1051/0004-6361:20065177. ISSN   0004-6361.
  8. ↑ information@eso.org. "A jellyfish and the ram". www.spacetelescope.org. Retrieved 18 April 2024.
  9. ↑ 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. (1 March 2016). "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.
  10. ↑ "Hubble Spots a Galaxy with Tendrils - NASA Science". science.nasa.gov. Retrieved 26 July 2024.
  11. ↑ Poggianti, Bianca M.; Gullieuszik, Marco; Tonnesen, Stephanie; Moretti, Alessia; Vulcani, Benedetta; Radovich, Mario; Jaffé, Yara; Fritz, Jacopo; Bettoni, Daniela; Franchetto, Andrea; Fasano, Giovanni; Bellhouse, Callum; Omizzolo, Alessandro (1 February 2019). "GASP XIII. Star formation in gas outside galaxies". Monthly Notices of the Royal Astronomical Society. 482 (4): 4466–4502. arXiv: 1811.00823 . Bibcode:2019MNRAS.482.4466P. doi: 10.1093/mnras/sty2999 . ISSN   0035-8711.
  12. ↑ Moretti, A.; Paladino, R.; Poggianti, B. M.; D'Onofrio, M.; Bettoni, D.; Gullieuszik, M.; Jaffé, Y. L.; Vulcani, B.; Fasano, G.; Fritz, J.; Torstensson, K. (1 October 2018). "GASP – X. APEX observations of molecular gas in the discs and in the tails of ram-pressure stripped galaxies". Monthly Notices of the Royal Astronomical Society. 480 (2): 2508–2520. arXiv: 1803.06183 . Bibcode:2018MNRAS.480.2508M. doi: 10.1093/mnras/sty2021 . ISSN   0035-8711.
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