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Messier 61
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== 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">{{cite web |title=Galaxy On Line Database Milano Network (GOLDMine) |url=http://goldmine.mib.infn.it/ |access-date=2012-08-06 |archive-url=https://web.archive.org/web/20120603100014/http://goldmine.mib.infn.it/ |archive-date=2012-06-03 |url-status=dead }}</ref><ref name="VirgoAtlas">{{cite web |title=The Virgo Cluster |url=http://www.atlasoftheuniverse.com/galgrps/vir.html |access-date=2013-04-06 }}</ref> The [[Galaxy morphological classification|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"> {{cite journal | last=de Vaucouleurs |first=Gérard | title=Revised Classification of 1500 Bright Galaxies | journal=Astrophysical Journal Supplement | date=April 1963 | volume=8 | page=31 | doi=10.1086/190084 |bibcode=1963ApJS....8...31D }}</ref> It has an [[active galactic nucleus]]<ref name="Jiménez-Bailón2003"> {{cite journal |last1=Jiménez-Bailón |first1=E. |last2=Santos-Lleó |first2=M. |last3=Mas-Hesse |first3=J. M. |last4=Guainazzi |first4=M. |last5=Colina |first5=L. |last6=Cerviño |first6=M. |last7=González Delgado |first7=Rosa M. |date=2003 |title=Nuclear Activity and Massive Star Formation in the Low-Luminosity Active Galactic Nucleus NGC 4303: Chandra X-Ray Observations |journal=[[The Astrophysical Journal]] |volume=593 |issue=1 |pages=127–141 |doi=10.1086/376554 |bibcode=2003ApJ...593..127J |arxiv=astro-ph/0304465 |s2cid=12969809 }}</ref> and is classified as a [[starburst galaxy]] containing a [[Super star cluster|massive]] [[nuclear star cluster]] with an estimated mass of 10<sup>5</sup> [[solar mass]]es and an age of 4 million years,<ref name="Colina2002">{{cite journal |last1=Colina |first1=L. |last2=Gonzalez Delgado |first2=R. |last3=Mas-Hesse|first3=J. Miguel |last4=Leitherer |first4=C. |last5=Jimenez Bailon |first5=E. |date=2002 |title=Detection of a Super-Star Cluster as the Ionizing Source in the Low-Luminosity Active Galactic Nucleus NGC 4303 |journal=[[The Astrophysical Journal]] |volume=579 |issue=2 |pages=545–553 |doi=10.1086/342839 |bibcode=2002ApJ...579..545C|doi-access=free |hdl=10261/191615 |hdl-access=free }}</ref> as well as a central candidate [[supermassive black hole]] weighing around {{solar mass|5×10<sup>6</sup>}} solar masses.<ref name="Pastorini2007">{{cite journal |last1=Pastorini |first1=G. |last2=Marconi |first2=A. |last3=Capetti |first3=A. |last4=Axon |first4=D. J. |last5=Alonso-Herrero |first5=A.|author5-link=Almudena Alonso-Herrero |last6=Atkinson |first6=J. |last7=Batcheldor |first7=D. |last8=Carollo |first8=C. M. | author-link8 = C. Marcella Carollo|last9=Collett |first9=J. |last10=Dressel |first10=L. |last11=Hughes |first11=M. A. |last12=Macchetto |first12=D. |last13=Maciejewski |first13=W. |last14=Sparks |first14=W. |last15=van der Marel |first15=R. |date=2007 |title=Supermassive black holes in the Sbc spiral galaxies NGC 3310, NGC 4303 and NGC 4258 |journal=[[Astronomy and Astrophysics]] |volume=469 |issue=2 |pages=405–423 |doi=10.1051/0004-6361:20066784 |bibcode=2007A&A...469..405P |arxiv=astro-ph/0703149|s2cid=849621 }}</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 [[nebula]]e appears across M61's disk.<ref name="Koopmann2004"> {{cite journal |last1=Koopmann |first1=R. |last2=Kenney |first2=J. D. P. |date=2004 |title=Hα Morphologies and Environmental Effects in Virgo Cluster Spiral Galaxies |journal=The Astrophysical Journal |volume=613 |issue=2 |pages=866–885 |bibcode=2004ApJ...613..866K |doi=10.1086/423191 |arxiv=astro-ph/0406243 |s2cid=17519217 }}</ref> Unlike most [[Hubble classification|late-type spiral galaxies]] within the Virgo Cluster, M61 shows an unusual abundance of [[neutral hydrogen]] (H I).<ref name="Kenney1986"> {{cite journal |last1=Kenney |first1=J. D. |last2=Young |first2=J. S. |date=1986 |title=CO in H I-deficient Virgo cluster spiral galaxies |journal=[[The Astrophysical Journal Letters]] |volume=301 |pages=L13–L17 |doi=10.1086/184614 |bibcode=1986ApJ...301L..13K|doi-access=free }}</ref>
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