Jump to content

Messier 110

Coordinates: Sky map 00h 40m 22.1s, +41° 41′ 07″
From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by TowardsTheLight (talk | contribs) at 08:33, 26 June 2017 (Removed the edit of 23:40, 19 May 2017, by‎ 77.96.57.97 that reintroduced an incorrect name (probable vandalism)). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Template:Galaxybox begin Template:Galaxybox image Template:Galaxybox observe Template:Galaxybox character Template:Galaxybox astrometry Template:Galaxybox catalog Template:Galaxybox reference Template:Galaxybox end

In this image of the Andromeda Galaxy, Messier 110 is to the bottom-right of the center.

Messier 110, also known as 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 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, including one discovered in 1999 by Johnson and Modjaz,[4] and another detected in 2002, by Nakano and Sumoto. The latter, designated EQ J004015.8+414420, had also been captured in images taken by the Sloan Digital Sky Survey (SDSS) in October, 2002. [5]

Unlike M32, NGC205 does not (as of 2005) show evidence for a supermassive black hole at its center.[6]

See also

References

  1. ^ a b A. Sandage; J. Bedke (1994). Carnegie Atlas of Galaxies. Carnegie Institution of Washington. ISBN 0-87279-667-1.
  2. ^ a b K.G. Jones (1991). Messier's Nebulae and Star Clusters (2nd ed.). Cambridge University Press. ISBN 0-521-37079-5.
  3. ^ K.G. Jones (1967). "Some New Notes on Messier's Catalogue". Sky & Telescope. 33: 156–158. Bibcode:1967S&T....33..156J.
  4. ^ 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.
  5. ^ ""Forum di Astronomia Amatoriale Italiano"".
  6. ^ 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.