Messier 61

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Messier 61 (also known as M61, NGC 4303, or the Swelling Spiral Galaxy) is an intermediate barred spiral galaxy in the Virgo Cluster of galaxies. It was first discovered by Barnaba Oriani on May 5, 1779, six days before Charles Messier discovered the same galaxy. Messier had observed it on the same night as Oriani but had mistaken it for a comet.<ref name="SEDS">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> Its distance has been estimated to be 45.61 million light years from the Milky Way Galaxy. It is a member of the M61 Group of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.<ref name="atlas universe">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>

Properties

M61 is one of the largest members of Virgo Cluster, and belongs to a smaller subgroup known as the S Cloud.<ref name="GOLDMine">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref><ref name="VirgoAtlas">{{#invoke:citation/CS1|citation |CitationClass=web }}</ref> The morphological classification of SAB(rs)bc<ref name="ned" /> indicates a weakly-barred spiral (SAB) with the suggestion of a ring structure (rs) and moderate to loosely wound spiral arms.<ref name="Class"> Template:Cite journal</ref> It has an active galactic nucleus<ref name="Jiménez-Bailón2003"> Template:Cite journal</ref> and is classified as a starburst galaxy containing a massive nuclear star cluster with an estimated mass of 1 million solar masses (Template:Solar mass) and an age of 4 million years,<ref name="Colina2002">Template:Cite journal</ref> as well as a central candidate supermassive black hole weighing around Template:Solar mass.<ref name="Pastorini2007">Template:Cite journal</ref> It cohabits with an older massive star cluster as well as a likely older starburst.<ref name=Colina2002/> Evidence of significant star formation and active bright nebulae appears across M61's disk.<ref name="Koopmann2004"> Template:Cite journal</ref> Unlike most late-type spiral galaxies within the Virgo Cluster, M61 shows an unusual abundance of neutral hydrogen (H I).<ref name="Kenney1986"> Template:Cite journal</ref>

Supernovae

Eight supernovae have been observed in M61, making it one of the most prodigious galaxies for such cataclysmic events.<ref>Supernovae which have been observed in Messier catalog galaxies</ref><ref name="eps_super"> {{#invoke:citation/CS1|citation |CitationClass=web }}</ref><ref name="SEDS" /> These include:

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  • SN 1961I (Type II, mag. 13) was discovered by Milton Humason on 3 June 1961.<ref>{{#invoke:citation/CS1|citation

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  • SN 1964F (Type II, mag. 14) was discovered by Leonida Rosino on 30 June 1964.<ref>{{#invoke:citation/CS1|citation

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  • SN 2008in (Type II, mag. 14.9) was discovered by Kōichi Itagaki on 26 December 2008.<ref>Template:Cite journal</ref><ref>{{#invoke:citation/CS1|citation

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See also

References

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