Messier 110
Template:Galaxybox begin Template:Galaxybox image Template:Galaxybox observe Template:Galaxybox character Template:Galaxybox astrometry Template:Galaxybox catalog Template:Galaxybox reference Template:Galaxybox end Messier 110 (also known as 'The Edward Young Star' and NGC 205) is a dwarf elliptical galaxy that is a satellite of the Andromeda Galaxy.[1] M110 contains some dust and hints of recent star formation, which is unusual for dwarf elliptical galaxies in general.[1]
History
Although Charles Messier never included the galaxy in his famous list, it was depicted by him, together with M32, on a drawing of the Andromeda galaxy; a label on the drawing indicates that Messier first observed NGC 205 on August 10, 1773.[2] The galaxy was independently discovered by Caroline Herschel on August 27, 1783; her brother William Herschel described her discovery in 1785.[2] The suggestion to assign the galaxy a Messier number was made by Kenneth Glyn Jones in 1967.[3]
A few novae have been detected in this galaxy. Notably one discovered in 1999 by Johnson and Modjaz,[4] and another detected in 2002, by Nakano and Sumoto. The latter one, designated EQ J004015.8+414420, had also been captured in images taken by the SDSS (Sloan Digital Sky Survey) in October, 2002. [5]
Unlike M32, NGC205 does not show evidence for a supermassive black hole at its center.[6]
See also
References
- ^ a b A. Sandage; J. Bedke (1994). Carnegie Atlas of Galaxies. Carnegie Institution of Washington. ISBN 0-87279-667-1.
- ^ a b K.G. Jones (1991). Messier's Nebulae and Star Clusters (2nd ed.). Cambridge University Press. ISBN 0-521-37079-5.
- ^ K.G. Jones (1967). "Some New Notes on Messier's Catalogue". Sky & Telescope. 33: 156–158. Bibcode:1967S&T....33..156J.
- ^ van den Bergh, S. (2000). "Updated Information on the Local Group". Publications of the Astronomical Society of the Pacific. 112 (770): 529–536. arXiv:astro-ph/0001040. Bibcode:2000PASP..112..529V. doi:10.1086/316548.
- ^ ""Forum di Astronomia Amatoriale Italiano"".
- ^ Valluri, M.; Ferrarese, L.; Merritt, D.; Joseph, C.J. (2005). "The Low End of the Supermassive Black Hole Mass Function: Constraining the Mass of a Nuclear Black Hole in NGC 205 via Stellar Kinematics". Astrophysical Journal. 628 (1): 137–152. arXiv:astro-ph/0502493. Bibcode:2005ApJ...628..137V. doi:10.1086/430752.
External links
- Messier 110 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SEDS: Elliptical Galaxy M110
- Fohring, Dora; Merrifield, Michael. "M110 – Dwarf Galaxy". Deep Space Videos. Brady Haran.
| Location | Andromeda Galaxy → Andromeda subgroup →
Local Group → Local Sheet → Virgo Supercluster → Laniakea Supercluster → Local Hole → Observable universe → Universe Each → may be read as "within" or "part of". | .jpg) |
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*It is uncertain whether these are companion galaxies of the Andromeda Galaxy | |
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