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Messier 88 (also known as M88 or NGC 4501) is a spiral galaxy about 50 to 60 million light-years away from Earth[3][4][5] in the constellation Coma Berenices. It was discovered by Charles Messier in 1781.

Messier 88
Spiral Galaxy Messier 88
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 31m 59.2s[1]
Declination+14° 25′ 14″[1]
Redshift0.007609
Helio radial velocity2281
Galactocentric velocity2235
Apparent magnitude (V)9.6[2]
Characteristics
TypeSA(rs)b, HII Sy2[1]
Apparent size (V)6.9 × 3.7 moa[1]
Other designations
NGC 4501, UGC 7675, PGC 41517, VCC 1401[1]

Properties


M88 is one of the fifteen Messier objects that belong to the nearby Virgo Cluster of galaxies. It is galaxy number 1401 in the Virgo Cluster Catalogue (VCC) of 2096 galaxies that are candidate members of the cluster.[6] M88 appears to be on or ending a highly elliptical orbit, currently on an approximate or direct course toward the cluster center, which is occupied by the giant elliptical galaxy M87. It is currently 0.3 to 0.48 million parsecs from the center and will come closest to the core in about 200 to 300 million years. Its motion through the intergalactic medium of its cluster is creating, as expected, ram pressure that is stripping away the outer region of neutral hydrogen. To date, this has been detected along the western, leading edge of the galaxy.[7]

This galaxy is inclined to the line of sight by 64°.[8] It is classified as an Sbc spiral, a status between Sb (medium-wound) and Sc (loosely wound) spiral arms. The spiralling arms are very regular and can be followed down to the galactic core.[9] The maximum rotation velocity of the gas is 241.6 ± 4.5 km/s.[10]

M88 is classified as a type 2 Seyfert galaxy, which means it produces narrow spectral line emission from highly ionized gas in the nucleus.[11] In the core region there is a central condensation with a 230 parsec diameter, which has two concentration peaks. This condensation is being fed by inflow from the spiral arms.[12] The supermassive black hole at the core of this galaxy has 107.9 solar masses, or about 80 million solar masses (M☉).[13]

In 1999, supernova 1999cl was discovered in this galaxy.[14]

Location of M88
Location of M88

See also



References


  1. "Results for NGC 4501". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 14 November 2006.
  2. "Messier 88". SEDS Messier Catalog. Retrieved 30 April 2022.
  3. "Object Information". 20 September 2009. Retrieved 26 December 2012.
  4. Nemiroff, R.; Bonnell, J., eds. (30 January 2010). "Messier 88". Astronomy Picture of the Day. NASA. Retrieved 26 December 2012.
  5. "M88". 29 June 2011. Retrieved 26 December 2012.
  6. Binggeli, B.; Sandage, A.; Tammann, G. A. (1985). "Studies of the Virgo Cluster. II – A catalog of 2096 galaxies in the Virgo Cluster area". Astronomical Journal. 90: 1681–1759. Bibcode:1985AJ.....90.1681B. doi:10.1086/113874.
  7. Vollmer, B.; et al. (2008). "Pre-peak ram pressure stripping in the Virgo cluster spiral galaxy NGC 4501". Astronomy & Astrophysics. 483 (1): 89–106. arXiv:0801.4874. Bibcode:2008A&A...483...89V. doi:10.1051/0004-6361:20078139. S2CID 15005390.
  8. Tully, R. B.; Fisher, J. R. (1977). "A new method of determining distances to galaxies". Astronomy & Astrophysics. 54 (3): 661–673. Bibcode:1977A&A....54..661T.
  9. Möllenhoff, C.; Heidt, J. (2001). "Surface photometry of spiral galaxies in NIR: Structural parameters of disks and bulges". Astronomy & Astrophysics. 368 (1): 16–37. Bibcode:2001A&A...368...16M. doi:10.1051/0004-6361:20000335.
  10. "Database for physics of galaxies". HyperLeda. Université de Lyon. Retrieved 16 September 2009.
  11. Sparke, L. S.; Gallagher, J. S. III (2007). Galaxies in the Universe: An Introduction. Cambridge University Press. ISBN 978-0-521-67186-6.
  12. Onodera, S.; Sofue, Y.; Koda, J.; Nakanishi, H.; Kohno, K. (2002). "CO (J=1-0) Observations of the Non-Barred Seyfert 2 Galaxy NGC 4501". In Ikeuchi, S.; Hearnshaw, J.; Hanawa, T. (eds.). Proceedings of the IAU 8th Asian-Pacific Regional Meeting. 8Th Asian-Pacific Regional Meeting. p. 199. Bibcode:2002aprm.conf..199O.
  13. 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.
  14. James, N. D. (1999). "Supernova 1999cl in NGC 4501 (M88)". Journal of the British Astronomical Association. 109 (4): 178. Bibcode:1999JBAA..109..178J.


Wikimedia Commons has media related to Messier 88.
Wikimedia Commons has media related to NGC 4501.


На других языках

[de] Messier 88

Messier 88 (auch als NGC 4501 bezeichnet) ist eine 9,6 mag helle Spiralgalaxie mit einer Flächenausdehnung von 6,8′ × 3,7′ im Sternbild Haar der Berenike (Coma Berenices) am Nordsternhimmel. In der Hubble-Sequenz wird dieser Galaxie der Typ Sb zugeordnet. Sie wurde am 18. März 1781 vom französischen Astronomen Charles Messier zusammen mit sieben anderen Galaxien des Virgo-Galaxienhaufens entdeckt. Die galaktische Ebene von M88 ist um etwa 30 Grad gegen die Sichtlinie geneigt, wodurch sie eine gewisse Ähnlichkeit gewinnt mit dem Andromedanebel, der ebenfalls vom Typ Sb ist.
- [en] Messier 88

[es] Galaxia espiral M88

Messier 88 (también conocido como M88 o NGC 4501) es una galaxia espiral a unos 49 millones de años luz en la constelación Coma Berenices. La galaxia es un miembro del cúmulo de Virgo, y una de las galaxias más grandes y brillantes de este, con una luminosidad comparable a la de la Galaxia de Andrómeda. Fue descubierta por Charles Messier en 1781.[cita requerida]

[ru] M 88 (галактика)

Messier 88 (англ. M 88, NGC 4501, рус. Мессье 88, другие обозначения — UGC 7675, MCG 3-32-59, ZWG 99.76, VCC 1401, PGC 41517) — спиральная галактика в созвездии Волосы Вероники.


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