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Virgo Cluster
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== Intracluster medium == As with many other rich galaxy clusters, Virgo's [[intracluster medium]] is filled with a hot, rarefied [[plasma (physics)|plasma]] at temperatures of 30 million [[kelvin]]s that emits [[X-Rays]].<ref name="Lea1982">{{cite journal | author=Lea, S. M. | author2=Mushotzky, R. | author3=Holt, S. S. | title=Einstein Observatory solid state spectrometer observations of M87 and the Virgo cluster | journal=Astrophysical Journal | date=1982 | issue=1 | volume=262 | pages=24–32 |bibcode = 1982ApJ...262...24L |doi = 10.1086/160392 | hdl=2060/19820026438 | s2cid=120960432 | hdl-access=free }}</ref> Within the intracluster medium (ICM) are found a large number of [[intergalactic star]]s<ref name="HST1997">{{cite journal | author=Ferguson, H. | title=Intergalactic Stars in the Virgo Cluster | journal=HST Proposal | date=1997 | bibcode=1997hst..prop.7411F| pages=7411 }}</ref><ref>{{Cite journal|last1=Ferguson|first1=Henry C.|last2=Tanvir|first2=Nial R.|last3=von Hippel|first3=Ted|date=January 1998|title=Detection of intergalactic red-giant-branch stars in the Virgo cluster|journal=Nature|language=En|volume=391|issue=6666|pages=461–463|doi=10.1038/35087|issn=0028-0836|arxiv=astro-ph/9801228|bibcode=1998Natur.391..461F|s2cid=4390832}}</ref> (up to 10% of the stars in the cluster),<ref name=Fergusonetal1998/> including some [[planetary nebula]]e.<ref name="Feldmeieretal1998">{{cite journal | author=Feldmeier, J. | author2=Ciardullo, R. | author3=Jacoby, G. | title=Intracluster Planetary Nebulae in the Virgo Cluster. I. Initial Results | journal=Astrophysical Journal | date=1998 | volume=503 | issue=1 | pages=109–117 |arxiv = astro-ph/9803062 |bibcode = 1998ApJ...503..109F |doi = 10.1086/305981 | s2cid=9761241 }}</ref> It is theorized that these were expelled from their home galaxies by [[Interacting galaxy|interactions with other galaxies]].<ref name="Fergusonetal1998">{{cite journal | author=Ferguson, Henry C. | author2=Tanvir, Nial R. | author3=von Hippel, Ted | title=Detection of intergalactic red-giant-branch stars in the Virgo cluster | journal=Nature | date=1998 | volume=391 | pages=461–463 |arxiv = astro-ph/9801228 |bibcode = 1998Natur.391..461F |doi = 10.1038/35087 | issue=6666 | s2cid=4390832 }}</ref> The ICM also contains some [[globular cluster]]s,<ref name="Takamiya2009">{{cite book | author=Takamiya, Marianne | author2=West, Michael | author3=Côté, Patrick | author4=Jordán, Andrés | author5=Peng, Eric | author6=Ferrarese, Laura | title=Globular Clusters – Guides to Galaxies | chapter=IGCs in the Virgo Cluster | journal=Globular Clusters – Guides to Galaxies, Eso Astrophysics Symposia, Volume | date=2009 | pages=361–365 | bibcode=2009gcgg.book..361T| doi=10.1007/978-3-540-76961-3_83 | series=Eso Astrophysics Symposia | isbn=978-3-540-76960-6 }}</ref><ref name="Durrell2010">{{cite journal | author=Durrell, Patrick R. | author2=Accetta, K. | author3=Feldmeier, J. J. | author4=Mihos, J. C. | author5=Ciardullo, R. | author6=Peng, E. W. | author7=Members of the NGVS team | title=Searching for Intracluster Globular Clusters in the Virgo Cluster | date=2010 | journal=Bulletin of the American Astronomical Society | volume=42 |pages=567 | bibcode=2010AAS...21547814D }}</ref><ref name="Park2010">{{cite journal | author=Lee, Myung Gyoon | author2=Park, Hong Soo | author3=Hwang, Ho Seong | title=Detection of a Large-Scale Structure of Intracluster Globular Clusters in the Virgo Cluster | journal=Science | date=2010 | volume=328 | pages=334– |arxiv = 1003.2499 |bibcode = 2010Sci...328..334L |doi = 10.1126/science.1186496 | issue=5976 | pmid=20223950 | s2cid=20743125 }}</ref> possibly stripped off [[dwarf galaxy|dwarf galaxies]],<ref name=Park2010/> and even at least one [[star formation]] [[H II region|region]].<ref name="Ortwin2002">{{cite journal | author=Gerhard, Ortwin | author2=Arnaboldi, Magda | author3=Freeman, Kenneth C. | author4=Okamura, Sadanori | title=Isolated Star Formation: A Compact H II Region in the Virgo Cluster | journal=The Astrophysical Journal | date=2002 | volume=580 | pages=L121–L124 |arxiv = astro-ph/0211341 |bibcode = 2002ApJ...580L.121G |doi = 10.1086/345657 | issue=2 | s2cid=8686119 }}</ref>
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