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From Wikipedia, the free encyclopedia

Messier 66
Phot-33c-03-fullres.jpg
A colour-composite image of M66.
Observation data (J2000 epoch)
ConstellationLeo
Right ascension11h 20m 15.026s[1]
Declination+12° 59′ 28.64″[1]
Redshift0.002425±0.000010[2] (696.3±12.7 km/s)[3]
Distance31 Mly (9.6 Mpc)[4]
Apparent magnitude (V)8.9[2]
Characteristics
TypeSABb[5]
Apparent size (V)9.1′ × 4.2′[6]
Notable featuresGalaxy in the Leo Triplet
Other designations
Arp 16, NGC 3627, PGC 34695, UGC 6346[7]
See also: Galaxy, List of galaxies

Messier 66 or M66, also known as NGC 3627, is an intermediate spiral galaxy in the equatorial constellation of Leo. It was discvered by French astronomer Charles Messier[8] on March 1, 1780, who described it as "very long and very faint".[9] This galaxy is a member of a small group of galaxies that includes M65 and NGC 3628, known as the Leo Triplet, or the M66 Group.[10] M65 and M66 make a popular pair for observers, being separated by only 20.[9]

M66 has a morphological classification of SABb,[5] indicating a spiral shape with a weak bar feature and loosely wound arms. The isophotal axis ratio is 0.32, indicating that it is being viewed at an angle.[5] M66 is receding from us with a heliocentric radial velocity of 696.3±12.7 km/s.[3] It lies 31[4] million light-years away and is about 95 thousand light-years across[11] with striking dust lanes and bright star clusters along sweeping spiral arms. As of 2018, five supernovae have been observed in M66: SN 2016cok,[12] 2009hd, 1997bs, 1989B, and 1973R.[13]

Gravitational interaction from its past encounter with neighboring NGC 3628 has resulted in an extremely high central mass concentration; a high molecular to atomic mass ratio; and a resolved non-rotating clump of H I material apparently removed from one of the spiral arms. The latter feature shows up visually as an extremely prominent and unusual spiral arm and dust lane structures as originally noted in the Atlas of Peculiar Galaxies.[14]

Gallery

References

  1. ^ a b Skrutskie, M. F.; et al. (February 2006), "The Two Micron All Sky Survey (2MASS)", The Astronomical Journal, 131 (2): 1163–1183, Bibcode:2006AJ....131.1163S, doi:10.1086/498708.
  2. ^ a b de Vaucouleurs, G.; et al. (1991), Third reference catalogue of bright galaxies, 9, New York: Springer-Verlag.
  3. ^ a b van den Bosch, Remco C. E.; et al. (May 2015), "Hunting for Supermassive Black Holes in Nearby Galaxies With the Hobby-Eberly Telescope", The Astrophysical Journal Supplement Series, 218 (1): 13, arXiv:1502.00632, Bibcode:2015ApJS..218...10V, doi:10.1088/0067-0049/218/1/10, 10.
  4. ^ a b Tully, R. Brent; et al. (August 2016), "Cosmicflows-3", The Astronomical Journal, 152 (2): 21, arXiv:1605.01765, Bibcode:2016AJ....152...50T, doi:10.3847/0004-6256/152/2/50, 50.
  5. ^ a b c Ann, H. B.; et al. (2015), "A Catalog of Visually Classified Galaxies in the Local (z ∼ 0.01) Universe", The Astrophysical Journal Supplement Series, 217 (2): 27–49, arXiv:1502.03545, Bibcode:2015ApJS..217...27A, doi:10.1088/0067-0049/217/2/27.
  6. ^ "NASA/IPAC Extragalactic Database", Results for NGC 3627, retrieved 2006-08-31.
  7. ^ "NGC 3627". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-12-02.
  8. ^ Frommert, Hartmut; Kronberg, Christine (June 15, 2016), Spiral Galaxy M66, retrieved 2018-12-03.
  9. ^ a b O'Meara, Stephen James (2014), Deep-Sky Companions: The Messier Objects, Deep-sky companions, Cambridge University Press, p. 248, ISBN 1107018374 It is recorded as discovered by Pierre Méchain, but apparently this is an error.
  10. ^ Adam, Len (2018), Imaging the Messier Objects Remotely from Your Laptop, The Patrick Moore Practical Astronomy Series, Springer, p. 290, ISBN 3319653857
  11. ^ Per the small angle formula: 31 mly × tan( 9′.1 ) = ~82 kly. diameter
  12. ^ Sutaria, Firoza; Ray, Alak (June 2016), "No X-ray detection of SN2016cok by Swift XRT", The Astronomer's Telegram, 9189, Bibcode:2016ATel.9189....1S.
  13. ^ List of Supernovae, Central Bureau for Astronomical Telegrams, retrieved 9 September 2015
  14. ^ Zhang, Xiaolei; et al. (1993), "High-Resolution CO and H i Observations of the Interacting Galaxy NGC 3627", Astrophysical Journal, 418: 100, Bibcode:1993ApJ...418..100Z, doi:10.1086/173374.

External links

This page was last edited on 3 December 2018, at 17:02
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