Messier 86
Messier 86 (also known as M86 or NGC 4406) is a lenticular galaxy in the constellation Virgo. It was discovered by Charles Messier in 1781. M86 lies in the heart of the Virgo Cluster of galaxies and forms a most conspicuous group with another giant, Lenticular Galaxy M84. It displays the highest blue shift of all Messier objects, as it is approaching the Milky Way at 244 km/s. This is due to its falling towards the center of the Virgo cluster from the opposite side, which causes it to move in the direction of the Milky Way.[3]
References
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4406. http://nedwww.ipac.caltech.edu/. Retrieved 2006-11-14.
- ^ Jensen, Joseph B.; Tonry, John L.; Barris, Brian J.; Thompson, Rodger I.; Liu, Michael C.; Rieke, Marcia J.; Ajhar, Edward A.; Blakeslee, John P. (2003). "Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations". Astrophysical Journal 583 (2): 712–726. arXiv:astro-ph/0210129. Bibcode 2003ApJ...583..712J. doi:10.1086/345430.
- ^ Jacoby, G. H.; Kenney, J. D. P.; Tal, T.; Crowl, H. H.; Feldmeier, J. J.; Kenney; Tal; Crowl; Feldmeier (2005). "Imaging and Spectroscopy of Large Scale H-alpha Filaments in M86". Bulletin of the American Astronomical Society 37: 1392. Bibcode 2005AAS...20713806J.
External links
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Flamsteed |
- 1 (ω)
- 2 (ξ)
- 3 (ν)
- 4 (A¹)
- 5 (β, Zavijava)
- 6 (A²)
- 7 (b)
- 8 (π)
- 9 (ο)
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- 15 (η, Zaniah)
- 16 (c)
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- 21 (q)
- 25 (f)
- 26 (χ)
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- 29 (γ, Porrima)
- 30 (ρ)
- 31 (d¹)
- 32 (d²)
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- 40 (ψ)
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- 43 (δ, Auva)
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- 47 (ε, Vindemiatrix)
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- 59 (e)
- 60 (σ)
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- 67 (α, Spica)
- 68 (i)
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- 74 (l, "el")
- 75
- 76 (h)
- 77
- 78 (o, small Latin "o")
- 79 (ζ, Heze)
- 80
- 82 (m)
- 83
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- 86
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- 89
- 90 (p)
- 92
- 93 (τ)
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- 98 (κ)
- 99 (ι, Syrma)
- 100 (λ, Khambalia)
- 102 (υ)
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- 105 (φ)
- 106
- 107 (μ, Rijl al Awwa)
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- 1 Ser (M)
- 2 Ser
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Galaxy cluster |
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Coordinates: 12h 26m 11.7s, +12° 56′ 46″
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See also |
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- Book:Messier objects
- Category:Messier objects
- Portal:Astronomy
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