Wikipedia

Virgo Cluster

TheVirgo Clusteris a largecluster of galaxieswhose center is53.8 ± 0.3Mly(16.5 ± 0.1Mpc)[2]away in theconstellationVirgo.Comprising approximately 1,300 (and possibly up to 2,000) member galaxies,[3]the cluster forms the heart of the largerVirgo Supercluster,of which theLocal Group(containing ourMilky Way galaxy) is a member. The Local Group actually experiences the mass of the Virgo Supercluster as theVirgocentric flow.It is estimated that the Virgo Cluster's mass is 1.2×1015M☉out to 8 degrees of the cluster's center or a radius of about 2.2 Mpc.[4]

Virgo Cluster
Virgo Cluster showing the diffuse light between membergalaxies.Messier 87is the largest galaxy (lower left).
Observation data (EpochJ2000)
Constellation(s)Virgo&Coma Berenices
Right ascension12h27m[1]
Declination+12° 43′[1]
Brightest memberMessier 49
Number of galaxies~1,500[1]
Parent structureVirgo Supercluster
Bautz–Morgan classificationIII[1]
Binding mass1015M☉

Many of the brighter galaxies in this cluster, including the giantelliptical galaxyMessier 87,were discovered in the late 1770s and early 1780s and subsequently included inCharles Messier's catalogue of non-cometary fuzzy objects. Described by Messier asnebulaewithout stars, their true nature was not recognized until the 1920s.[A]

The cluster subtends a maximum arc of approximately 8 degrees centered in the constellation Virgo. Although some of the cluster's most prominent members can be seen with smaller instruments, a 6-inch telescope will reveal about 160 of the cluster's galaxies on a clear night. Itsbrightest memberis theelliptical galaxyMessier 49;however its most famous member is the elliptical galaxyMessier 87,which is located in the center of the cluster.[6]

Characteristics

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The cluster is a fairlyheterogeneousmixture ofspiralandellipticalgalaxies.[7]As of 2004,it is believed that the spiral galaxies of the cluster are distributed in an oblongprolatefilament,approximately four times as long as it is wide, stretching along the line of sight from theMilky Way.[8]The elliptical galaxies are more centrally concentrated than the spiral galaxies.[9]

The cluster is an aggregate of at least three separatesubclumps:Virgo A,centered onM87,a second centered on the galaxyM86,andVirgo B,centered onM49,with some authors including aVirgo Csubcluster, centered on the galaxyM60as well as aLVC(Low Velocity Cloud) subclump, centered on the large spiral galaxyNGC 4216.[10]Notably, the giantelliptical galaxyM87 contains asupermassive black hole,whoseevent horizonwas observed by theEvent Horizon TelescopeCollaboration in 2019.[11][12]

Of all of the subclumps,Virgo A,formed by a mixture ofelliptical,lenticular,and (usually) gas-poorspiral galaxies,[13]is the dominant one, with a mass of approximately 1014M☉,which is approximately an order of magnitude larger than the other two subclumps.[14]

Turbulencemay prevent galaxy clusters from cooling (Chandra X-ray).

The three subgroups are in the process of merging to form a larger single cluster[14]and are surrounded by other smallergalaxy clouds,mostly composed of spiral galaxies, known asN Cloud,S Cloud,andVirgo Ethat are in the process of infalling to merge with them,[15]plus other farther isolated galaxies and galaxy groups (like the galaxy cloudComa I) that are also attracted by the gravity of Virgo to merge with it in the future.[16]This strongly suggests the Virgo cluster is a dynamically young cluster that is still forming.[15]

Other two nearby aggregations known asM Cloud,W Cloud,andW' Cloud[10]seem to be background systems independent of the main cluster.[15]

The large mass of the cluster is indicated by the highpeculiar velocitiesof many of its galaxies, sometimes as high as 1,600km/swith respect to the cluster's center.

The Virgo cluster lies within theVirgo Supercluster,and its gravitational effect slows down the nearby galaxies. The large mass of the cluster has the effect of slowing down the recession of the Local Group from the cluster by approximately ten percent.

Molecular gasses in Virgo Cluster has been swept away by a huge cosmic broom that is preventing nearby galaxies from birthing new stars. The actual cause of it has been a long standing mystery inastrophysics.According to scientists, it occurs because of the extreme environment of the Virgo Cluster.[17]

Intracluster medium

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As with many other rich galaxy clusters, Virgo'sintracluster mediumis filled with a hot, rarefiedplasmaat temperatures of 30 millionkelvinsthat emitsX-Rays.[18]Within the intracluster medium (ICM) are found a large number ofintergalactic stars[19][20](up to 10% of the stars in the cluster),[21]including someplanetary nebulae.[22]It is theorized that these were expelled from their home galaxies byinteractions with other galaxies.[21]The ICM also contains someglobular clusters,[23][24][25]possibly stripped offdwarf galaxies,[25]and even at least onestar formationregion.[26]

Galaxies

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Map of the Virgo Supercluster centered on theLocal Group(image diameter 200 Mly ≈ 60Mpc). The Virgo Cluster is visible in the center right of the image, at about 50 Mly from the Local Group.
Photograph of the Virgo Cluster with labelled galaxies

Below is a table of bright or notable objects in the cluster and their subunit (subcluster). Note that in some cases a galaxy may be considered in a different subunit by other researchers (sources:[10][15][27][28])

Column 1: The name of the galaxy.
Column 2: The right ascension for epoch 2000.
Column 3: The declination for epoch 2000.
Column 4: The blue apparent magnitude of the galaxy.
Column 5: The galaxy type: E=Elliptical, S0=Lenticular, Sa,Sb,Sc,Sd=Spiral, SBa,SBb,SBc,SBd=Barred spiral, Sm,SBm,Irr=Irregular.
Column 6: The angular diameter of the galaxy (arcminutes).
Column 7: The diameter of the galaxy (thousands of light years).
Column 8: The recessional velocity (km/s) of the galaxy relative to thecosmic microwave background.
Column 9: Subcluster where the galaxy is located.
Cluster members
Designation Coordinates(Epoch2000) Apparent
magnitude
(blue) 		Type Angular size Diameter
(kly) 		RV
(km/s) 		Subcluster
RA Dec
Messier 98 12 13.8 14 54 10.9 SBb 9.8′ 150 184 Virgo AorN Cloud
NGC 4216 12 15.9 13 09 10.9 SBb 7.9′ 120 459 Virgo A,N Cloud,orLVC.
Messier 99 12 18.8 14 25 10.4 Sc 5.4′ 80 2735 Virgo AorN Cloud
NGC 4262 12 19.5 14 53 12.4 S0 1.9′ 30 1683 Virgo A
NGC 4388 12 25.5 12 39 11.8 SAb 6.2′ 85 2845 Virgo A
Messier 61 12 21.9 04 28 10.2 SBbc 6.2′ 100 1911 S Cloud
Messier 100 12 22.9 15 49 10.1 SBbc 7.6′ 115 1899 Virgo A
Messier 84 12 25.1 12 53 10.1 E1 6.0′ 90 1239 Virgo A
Markarian's Chain
Messier 85 12 25.4 18 11 10.0 S0 7.1′ 105 1056 Virgo A
Messier 86 12 26.2 12 57 9.9 E3 10.2′ 155 37 Virgo Aor own subgroup.
Markarian's Chain
NGC 4435 12 27.7 13 05 11.7 S0 3.0′ 45 1111 Virgo A
NGC 4438 12 27.8 13 01 11.0 Sa 8.7′ 130 404 Virgo A
NGC 4450 12 28.5 17 05 10.9 Sab 5.1′ 80 2273 Virgo A
Messier 49 12 29.8 08 00 9.3 E2 9.8′ 150 1204 Virgo B
Messier 87 12 30.8 12 23 9.6 E0–1 9.8′ 980 1204 Virgo A
Messier 88 12 32.0 14 25 10.3 Sb 6.8′ 100 2599 Virgo A
NGC 4526 12 32.0 07 42 10.6 S0 7.1′ 105 931 Virgo B
NGC 4527 12 34.1 02 39 12.4 Sb 4.6′ 69 1730 S Cloud
NGC 4536 12 34.4 02 11 11.1 SBbc 7.2′ 115 2140 S Cloud
Messier 91 12 35.4 14 30 11.0 SBb 5.2′ 80 803 Virgo A
NGC 4546 12 35.5 -03 48 11.3 S0 2.3' 30 1054 S Cloud
NGC 4550 12 35.5 12 13 12.5 S0 3.2′ 50 704 Virgo A
Messier 89 12 35.7 12 33 10.7 E0 5.0′ 75 628 Virgo A
NGC 4567 12 36.5 11 15 12.1 Sbc 2.8′ 40 2588 Virgo A
NGC 4568 12 36.6 11 14 11.7 Sbc 4.4′ 65 2578 Virgo A
Messier 90 12 36.8 13 10 10.2 SBab 10.5′ 160 87 Virgo A
NGC 4571 12 36.9 14 13 11.9 Sc 3.7′ 55 659 Virgo A
Messier 58 12 37.7 11 49 10.6 SBb 5.6′ 85 1839 Virgo A
Messier 59 12 42.9 11 39 10.8 E5 5.0′ 75 751 Virgo AorVirgo E
Messier 60 12 43.7 11 33 9.8 E2 7.2′ 110 1452 Virgo A,Virgo E,orVirgo C
NGC 4651 12 43.7 16 24 11.4 Sc 4.0′ 60 1113
NGC 4654 12 43.9 13 08 11.1 SBc 5.0′ 75 1349 Virgo A

Fainter galaxies within the cluster are usually known by their numbers in the Virgo Cluster Catalog, particularly members of the numerous dwarf galaxy population.[29]

See also

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Notes

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  1. ^Following the entry for M91 in the Connoissance des Temps for 1784, Messier added the following note:
    The constellation of Virgo, & especially the northern Wing is one of the constellations which encloses the most Nebulae: this Catalog contains thirteen which have been determined: viz. Nos. 49, 58, 59, 60, 61, 84, 85, 86, 87, 88, 89, 90, & 91. All these nebulae appear to be without stars: one can see them only in a very good sky, & near their meridian passage. Most of these nebulae have been pointed to me by Mr. Méchain.[5]

References

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  1. ^abcd"NASA/IPAC Extragalactic Database".Results for Virgo Cluster.Retrieved2006-10-19.
  2. ^Mei, Simona; Blakeslee, John P.; Côté, Patrick; Tonry, John L.; West, Michael J.; Ferrarese, Laura; Jordán, Andrés; Peng, Eric W.; Anthony, André; Merritt, Davi (2007). "The ACS Virgo Cluster Survey. XIII. SBF Distance Catalog and the Three-dimensional Structure of the Virgo Cluster".The Astrophysical Journal.655(1): 144–162.arXiv:astro-ph/0702510.Bibcode:2007ApJ...655..144M.doi:10.1086/509598.S2CID16483538.
  3. ^"Virgo Cluster".Cosmos.Swinburne University of Technology.
  4. ^Fouqué, P.; Solanes, J. M.; Sanchis, T.; Balkowski, C. (2001). "Structure, mass and distance of the Virgo cluster from a Tolman-Bondi model".Astronomy and Astrophysics.375(3): 770–780.arXiv:astro-ph/0106261.Bibcode:2001A&A...375..770F.doi:10.1051/0004-6361:20010833.S2CID10468717.
  5. ^"Messier 91 — Observations and Descriptions".SEDS.
  6. ^"Virgo Cluster | Messier Objects".www.messier-objects.com.9 August 2017.Retrieved2018-06-24.
  7. ^Côté, Patrick; Blakeslee, John P.; Ferrarese, Laura; Jordán, Andrés; Mei, Simona;Merritt, David;Milosavljević, Miloš; Peng, Eric W.; Tonry, John L.; et al. (July 2004). "The ACS Virgo Cluster Survey".The Astrophysical Journal.153(1): 223–242.arXiv:astro-ph/0404138.Bibcode:2004ApJS..153..223C.doi:10.1086/421490.S2CID18021414.
  8. ^M. Fukugita; S. Okamura; N. Yasuda (1993). "Spatial distribution of spiral galaxies in the Virgo Cluster from the Tully-Fisher relation".Astrophysical Journal.412:L13–L16.Bibcode:1993ApJ...412L..13F.doi:10.1086/186928.
  9. ^"Virgo Cluster".ned.ipac.caltech.edu.Retrieved2018-06-24.
  10. ^abcBoselli, A.; Voyer, E.; Boissier, S.; Cucciati, O.; Consolandi, G.; Cortese, L.; Fumagalli, M.; Gavazzi, G.; Heinis, S.; Roehlly, Y.; Toloba, E. (2014). "The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). IV. The role of the cluster environment on galaxy evolution".Astronomy & Astrophysics.570:A69.arXiv:1407.4986.Bibcode:2014A&A...570A..69B.doi:10.1051/0004-6361/201424419.S2CID119244700.A69.
  11. ^Event Horizon Telescope Collaboration; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Asada, Keiichi; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Balokovic, Mislav; Barrett, John; Bintley, Dan (2019-04-01)."First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole".The Astrophysical Journal Letters.875(1): L1.arXiv:1906.11238.Bibcode:2019ApJ...875L...1E.doi:10.3847/2041-8213/ab0ec7.
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  14. ^abThe Virgo Super Cluster: home of M87(with frames)
  15. ^abcdGavazzi, G.; Boselli, A.; Scodeggio, M.; Pierini, D.; Belsole, E. (1999)."The 3D structure of the Virgo cluster from H-band Fundamental Plane and Tully-Fisher distance determinations".Monthly Notices of the Royal Astronomical Society.304(3): 595–610.arXiv:astro-ph/9812275.Bibcode:1999MNRAS.304..595G.doi:10.1046/j.1365-8711.1999.02350.x.S2CID41700753.
  16. ^Tully, R. B.; Shaya, E. J. (1984)."Infall of galaxies into the Virgo cluster and some cosmological constraints".Astrophysical Journal.281:31–55.Bibcode:1984ApJ...281...31T.doi:10.1086/162073.
  17. ^Brown, Toby; Wilson, Christine D.; Zabel, Nikki; Davis, Timothy A.; Boselli, Alessandro; Chung, Aeree; Ellison, Sara L.; Lagos, Claudia D. P.; Stevens, Adam R. H.; Cortese, Luca; Bahé, Yannick M. (2021-12-01)."VERTICO: The Virgo Environment Traced In CO Survey".The Astrophysical Journal Supplement Series.257(2): 21.arXiv:2111.00937.Bibcode:2021ApJS..257...21B.doi:10.3847/1538-4365/ac28f5.ISSN0067-0049.S2CID240354399.
  18. ^Lea, S. M.; Mushotzky, R.; Holt, S. S. (1982). "Einstein Observatory solid state spectrometer observations of M87 and the Virgo cluster".Astrophysical Journal.262(1): 24–32.Bibcode:1982ApJ...262...24L.doi:10.1086/160392.hdl:2060/19820026438.S2CID120960432.
  19. ^Ferguson, H. (1997). "Intergalactic Stars in the Virgo Cluster".HST Proposal:7411.Bibcode:1997hst..prop.7411F.
  20. ^Ferguson, Henry C.; Tanvir, Nial R.; von Hippel, Ted (January 1998). "Detection of intergalactic red-giant-branch stars in the Virgo cluster".Nature.391(6666): 461–463.arXiv:astro-ph/9801228.Bibcode:1998Natur.391..461F.doi:10.1038/35087.ISSN0028-0836.S2CID4390832.
  21. ^abFerguson, Henry C.; Tanvir, Nial R.; von Hippel, Ted (1998). "Detection of intergalactic red-giant-branch stars in the Virgo cluster".Nature.391(6666): 461–463.arXiv:astro-ph/9801228.Bibcode:1998Natur.391..461F.doi:10.1038/35087.S2CID4390832.
  22. ^Feldmeier, J.; Ciardullo, R.; Jacoby, G. (1998). "Intracluster Planetary Nebulae in the Virgo Cluster. I. Initial Results".Astrophysical Journal.503(1): 109–117.arXiv:astro-ph/9803062.Bibcode:1998ApJ...503..109F.doi:10.1086/305981.S2CID9761241.
  23. ^Takamiya, Marianne; West, Michael; Côté, Patrick; Jordán, Andrés; Peng, Eric; Ferrarese, Laura (2009). "IGCs in the Virgo Cluster".Globular Clusters - Guides to Galaxies.Eso Astrophysics Symposia. pp. 361–365.Bibcode:2009gcgg.book..361T.doi:10.1007/978-3-540-76961-3_83.ISBN978-3-540-76960-6.{{cite book}}:|journal=ignored (help)
  24. ^Durrell, Patrick R.; Accetta, K.; Feldmeier, J. J.; Mihos, J. C.; Ciardullo, R.; Peng, E. W.; Members of the NGVS team (2010). "Searching for Intracluster Globular Clusters in the Virgo Cluster".Bulletin of the American Astronomical Society.42:567.Bibcode:2010AAS...21547814D.
  25. ^abLee, Myung Gyoon; Park, Hong Soo; Hwang, Ho Seong (2010). "Detection of a Large-Scale Structure of Intracluster Globular Clusters in the Virgo Cluster".Science.328(5976): 334–.arXiv:1003.2499.Bibcode:2010Sci...328..334L.doi:10.1126/science.1186496.PMID20223950.S2CID20743125.
  26. ^Gerhard, Ortwin; Arnaboldi, Magda; Freeman, Kenneth C.; Okamura, Sadanori (2002). "Isolated Star Formation: A Compact H II Region in the Virgo Cluster".The Astrophysical Journal.580(2): L121–L124.arXiv:astro-ph/0211341.Bibcode:2002ApJ...580L.121G.doi:10.1086/345657.S2CID8686119.
  27. ^"Galaxy On Line Database Milano Network".GOLDMine.Retrieved2012-08-06.
  28. ^"The Virgo Cluster".Retrieved2013-04-06.
  29. ^Binggeli, Bruno;Sandage, Allan;Tammann, Gustav(1985). "Studies of the Virgo Cluster. II – A Catalog of 2096 Galaxies in the Virgo Cluster Area".Astronomical Journal.90.American Astronomical Society:1681–1759.Bibcode:1985AJ.....90.1681B.doi:10.1086/113874.
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