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Messier 58

Coordinates:Sky map12h 37m 43.522s, +11° 49′ 05.498″
From Wikipedia, the free encyclopedia
Galaxy in the constellation Virgo
For the motorway, seeM58 motorway.
Messier 58
Observation data (J2000epoch)
ConstellationVirgo[1]
Right ascension12h 37m 43.522s[2]
Declination+11° 49′ 05.498″[2]
Redshift0.00506[2][3]
Heliocentric radial velocity1517 ± 1km/s[2][3]
Distance21 megaparsecs (68 million light-years)[2][4]
Apparent magnitude (V)9.7[5]
Characteristics
TypeSAB(rs)b;
LINER[6]Sy 1.9[2][7]
Size40.72 kiloparsecs (133,000 light-years)
diameter;2MASSK-band total isophote[2][8]
Apparent size (V)5.9 × 4.7[2]
Other designations
NGC 4579,UGC 7796,PGC 42168, VCC 1727,GC 3121[2]

Messier 58 (also known asM58 andNGC 4579) is anintermediate barred spiral galaxy with a weak inner ring structure located within theconstellationVirgo, approximately 68 millionlight-years away fromEarth.[9][10] It was discovered byCharles Messier onApril 15, 1779 and is one of four barred spiral galaxies that appear in Messier's catalogue.[11][12][13][14][15][Note 1] M58 is one of the brightest galaxies in theVirgo Cluster.[16][17] From 1779 it was arguably (though unknown at that time) the farthest known astronomical object[18] until the release of theNew General Catalogue in the 1880s and even more so the publishing ofredshift values in the 1920s.

Early observations

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Charles Messier discovered Messier 58, along with theelliptical galaxiesMessier 59 andMessier 60, on April 15, 1779.[14] M58 was reported on the chart of theComet of 1779 as it was almost on the same parallel as the starEpsilon Virginis.[11][19] Messier described M58 as a very faintnebula in Virgo which would disappear in the slightest amount of light he used to illuminate themicrometer wires.[11][20] This description was later contradicted byJohn Herschel's observations in 1833 where he described it as a very bright galaxy, especially towards the middle. Herschel's observations were also similar to the descriptions of bothJohn Dreyer andWilliam Henry Smyth who said that M58 was a bright galaxy, mottled, irregularly round and very much brighter toward the middle.[11]

Characteristics

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Aninfrared image of M58 taken by theSpitzer Space Telescope (SST)

Like many other spiral galaxies of the Virgo Cluster (e.g.Messier 90), Messier 58 is ananemic galaxy with lowstar formation activity concentrated within the galaxy's optical disk,[21] and relatively littleneutral hydrogen, also located inside its disk, concentrated in clumps,[22] compared with other galaxies of similarmorphological type. This deficiency of gas is believed to be caused byinteractions with Virgo'sintracluster medium.

Messier 58 has a low-luminosityactive galactic nucleus, where astarburst may be present[23] as well as asupermassive black hole with a mass of around 70 millionsolar masses.[24] It is also one of the very few galaxies known to possess a UCNR (ultra-compact nuclear ring), a series ofstar-forming regions located in a very small ring around the center of the galaxy.[25] This led to its being dubbed the "ring bearer galaxy" by thepopular astronomy YouTube program "Deep Sky videos".[18]

Supernovae

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Twosupernovae have been observed in the M58 galaxy:

See also

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Notes

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  1. ^The other barred spiral galaxies in Messier's catalogue areMessier 91,Messier 95 andMessier 109

References

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  1. ^Sinnott, R. W., ed. (1988).The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer. Sky Publishing Corporation and Cambridge University Press.ISBN 978-0-933346-51-2.
  2. ^abcdefghi"Results for object MESSIER 058".NASA/IPAC Extragalactic Database.NASA andCaltech. Retrieved6 December 2024.
  3. ^abKent, Brian R.; Giovanelli, Riccardo; Haynes, Martha P.; Martin, Ann M.;Saintonge, Amélie; Stierwalt, Sabrina; Balonek, Thomas J.; Brosch, Noah; Koopmann, Rebecca A. (2008)."The Arecibo Legacy Fast Alfa Survey. VI. Second HI Source Catalog of the Virgo Cluster Region".The Astronomical Journal.136 (2): 713.arXiv:0806.3237.Bibcode:2008AJ....136..713K.doi:10.1088/0004-6256/136/2/713.
  4. ^Ruiz-Lapuente, Pilar (1996)."The Hubble Constant from 56Co-powered Nebular Candles".The Astrophysical Journal.465.arXiv:astro-ph/9604044.Bibcode:1996ApJ...465L..83R.doi:10.1086/310155.
  5. ^"Messier 58".SEDS Messier Catalog. Retrieved29 April 2022.
  6. ^Véron-Cetty, M. -P.; Véron, P. (2006)."A catalogue of quasars and active nuclei: 12th edition".Astronomy and Astrophysics.455 (2): 773.Bibcode:2006A&A...455..773V.doi:10.1051/0004-6361:20065177.
  7. ^Panessa, F.; Bassani, L. (2002)."Unabsorbed Seyfert 2 galaxies".Astronomy and Astrophysics.394 (2): 435.arXiv:astro-ph/0208496.Bibcode:2002A&A...394..435P.doi:10.1051/0004-6361:20021161.
  8. ^Jarrett, T. H.; Chester, T.; Cutri, R.; Schneider, S. E.; Huchra, J. P. (2003)."The 2MASS Large Galaxy Atlas".The Astronomical Journal.125 (2): 525.Bibcode:2003AJ....125..525J.doi:10.1086/345794.
  9. ^"Messier 58 Galaxy"(PDF).Solarius. Archived fromthe original(PDF) on 2010-10-11. Retrieved2010-02-09.
  10. ^"M 58".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2010-02-23.
  11. ^abcd"Messier 58: Observations and Descriptions".SEDS. Retrieved2010-02-23.
  12. ^Burnham, Robert Jr (1978).Burnham's Celestial Handbook: Volume Three, Pavo Through Vulpecula. Dover. pp. 2086–2088.ISBN 978-0-486-23673-5.
  13. ^Liller, William (1992).The Cambridge guide to astronomical discovery. Cambridge University Press. p. 29.ISBN 978-0-521-41839-3.
  14. ^abcde"Messier 58".SEDS. Retrieved2010-02-23.
  15. ^"Oceanside Photo and Telescope". Archived fromthe original on 2011-07-24. Retrieved2010-02-28.
  16. ^"Messier Object 58". Archived fromthe original on 1996-12-25. Retrieved2006-11-18.
  17. ^"Messier Catalog M51–M60".SEASKY. Retrieved2010-02-28.
  18. ^abSmethurst, Dr Rebecca; Haran, Brady (7 February 2018)."The Ring Bearer Galaxy (M58) – Deep Sky Videos".Deep Sky Videos. Brady Haran and University of Nottingham. Retrieved7 February 2018.
  19. ^"Charles Messier's Catalog of Nebulae and Star Clusters".SEDS: Charles Messier's Catalog. Retrieved2010-02-23.
  20. ^"Catalog of Nebulae and Star Clusters".SEDS: Observed at Paris by M. Messier. Retrieved2010-02-23.
  21. ^Koopmann, R. A.; Kenney, J. D. P. (2004). "Hα Morphologies and Environmental Effects in Virgo Cluster Spiral Galaxies".Astrophysical Journal.613 (2):866–885.arXiv:astro-ph/0406243.Bibcode:2004ApJ...613..866K.doi:10.1086/423191.S2CID 17519217.
  22. ^Cayatte, V.; van Gorkom, J. H.; Balkowski, C.; Kotanyi, C. (1990)."VLA observations of neutral hydrogen in Virgo Cluster galaxies. I – The Atlas".The Astronomical Journal.100:604–634.Bibcode:1990AJ....100..604C.doi:10.1086/115545.
  23. ^Contini, Marcella (2004)."The complex structure of low-luminosity active galactic nuclei: NGC 4579".Monthly Notices of the Royal Astronomical Society.354 (3):675–683.arXiv:astro-ph/0407379.Bibcode:2004MNRAS.354..675C.doi:10.1111/j.1365-2966.2004.08222.x.S2CID 16380554.
  24. ^Merloni, Andrea; Heinz, Sebastian;di Matteo, Tiziana (2003). "A Fundamental Plane of black hole activity".Monthly Notices of the Royal Astronomical Society.345 (4):1057–1076.arXiv:astro-ph/0305261.Bibcode:2003MNRAS.345.1057M.doi:10.1046/j.1365-2966.2003.07017.x.S2CID 14310323.
  25. ^Comerón, S.; Knapen, J. H.; Beckman, J. E. (2008). "Discovery of Four New Ultra-compact Nuclear Rings in Three Spiral Galaxies".Pathways Through an Eclectic Universe. ASP Conference Series. Vol. 390. p. 172.Bibcode:2008ASPC..390..172C.
  26. ^Kosai, H.; Ikeya, K.; Evans, R. O.; Bryan, J.; Wheeler, J. C.; Cochran, A.; Barker, E.; Schlegel, E. M.; Peters, J. (1988)."Supernova 1988A in M58".International Astronomical Union Circular (4533): 1.Bibcode:1988IAUC.4533....1K.
  27. ^"SN 1988A".Transient Name Server.IAU. Retrieved6 December 2024.
  28. ^Kharadze, E. K.; Pskovsky, Yu. P.; Kimeridze, G. N.; Turatto, M.; Cappellaro, E.; La Franca, F.; Filippenko, A. V.; Dey, A. (1989)."Supernova 1989M in NGC 4579".International Astronomical Union Circular (4802): 1.Bibcode:1989IAUC.4802....1K.
  29. ^"SN 1989M".Transient Name Server.IAU. Retrieved6 December 2024.

External links

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