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Local Sheet

From Wikipedia, the free encyclopedia
Nearby small galaxy filement
Local Sheet
The Local Sheet on the top view within 10 million light-years from Earth, including the Local Group and other nearby giant galaxies.
A portion of the Local Sheet, the Council of Giants, on the top view within 10 million light-years from Earth, including theLocal Group and other nearby giant galaxies.
Observation data (EpochJ2000)
Number of galaxies14 (giant galaxies)[1]
Parent structureLocal Volume[1]
Major axis33.9 Mly (10.4 Mpc)[1]
Minor axis1.52 Mly (0.465 Mpc)[1]
Velocity dispersion47 km/s[1]
Distance420,700 ly (129 kpc) (center)[1]
ICM temperature7.3×105 K[1]
Binding mass1.6×1013[1] M
Other designations
Local Street, Coma–Sculptor Cloud[1]
The 14 major galaxies, including Milky Way and Andromeda Galaxies, of the Local Sheet

TheLocal Sheet or theComa–Sculptor Cloud is a nearbygalaxy filament and an extragalactic region of space where theMilky Way, the members of theLocal Group, and othergalaxies share a similarpeculiar velocity.[2] This region lies within a diameter of about 10.4megaparsecs (34 millionlight-years; 3.2×1020kilometres), 465kiloparsecs (1.52 millionlight-years; 1.43×1019kilometres) thick,[1] and galaxies beyond that distance show markedly different velocities.[3] The Local Group has only a relatively small peculiar velocity of66 km⋅s−1 with respect to the Local Sheet. Typical velocity dispersion of galaxies is only40 km⋅s−1 in the radial direction.[2] Nearly all nearby bright galaxies belong to the Local Sheet.[4] The Local Sheet is part of theLocal Volume and is in theVirgo Supercluster (Local Supercluster).[1] The Local Sheet forms a wall of galaxies delineating one boundary of theLocal Void.[5]

A significant component of the mean velocity of the galaxies in the Local Sheet appears as the result of thegravitational attraction of theVirgo Cluster of galaxies, resulting in a peculiar motion ~185 km⋅s−1 toward the cluster.[2] A second component is directed away from the center of theLocal Void; an expanding region of space spanning an estimated 45 Mpc (150 Mly) that is only sparsely populated with galaxies.[3] This component has a velocity of259 km⋅s−1.[2] The Local Sheet is inclined 8° from theLocal Supercluster (Virgo Supercluster).[1]

The so-calledCouncil of Giants is a ring of twelve large galaxies surrounding the Local Group in the Local Sheet, with a radius of 3.746 Mpc (12.22 Mly) and its center located at 810 kpc (2.6 Mly) away from theSun.[1] Ten of these arespirals, while the remaining two areellipticals. The two ellipticals (Maffei 1 andCentaurus A) lie on opposite sides of the Local Group.

Galaxies in the "Council of Giants"[1]
Catalog IDNameConstellationDistance (Mly)Stellar mass *
NGC 253Sculptor GalaxySculptor1110.805
PGC 9892Maffei 1Cassiopeia1110.928
PGC 10217Maffei 2Cassiopeia1110.493
IC 342 Camelopardalis1110.302
NGC 3031M 81Ursa Major1210.905
NGC 3034M 82Ursa Major1110.573
NGC 4736M 94Canes Venatici1510.458
NGC 4826M 64Coma Berenices1610.496
NGC 5236M 83Hydra1610.642
NGC 5128Centaurus ACentaurus1111.169
NGC 4945 Centaurus1210.528
ESO 97-G13Circinus GalaxyCircinus1410.559
A portion of the Local Sheet within a map of 8 million light-years from Earth, including theLocal Group and some other nearby galaxies.

* The mass is given as the logarithm (base unspecified) of the mass insolar masses.

Location

[edit]

The Local Sheet is the co-moving part of the Coma-Sculptor Cloud,[6] which was identified and described in 1987 by astronomerBrent Tully with colleagueRichard Fisher in his bookThe Nearby Galaxies Atlas asCloud 14.[7] It is a huge 10 Mpc (33 Mly) prolate,[8] filament[9][10][2][8] and is mostly host to late-type galaxies, in contrast to theVirgo Cluster, in which more than half of the giant galaxies are early-type galaxies.[11]

Tully maintains that the Coma-Sculptor Cloud and the Local Sheet do not quite overlap,[2] as the Local Sheet comprises only the co-moving part of the Coma-Sculptor Cloud.[6] McCall considers the two terms synonymous, referring to one and the same region.[1]

See also

[edit]

References

[edit]
  1. ^abcdefghijklmnoMcCall, Marshall L. (29 April 2013)."A Council of Giants".Monthly Notices of the Royal Astronomical Society.440 (1) (published 10 March 2014):405–426.arXiv:1403.3667.Bibcode:2014MNRAS.440..405M.doi:10.1093/mnras/stu199.
  2. ^abcdefTully, R. Brent; Shaya, Edward J.; Karachentsev, Igor D.;Courtois, Hélène M.; Kocevski, Dale D.; Rizzi, Luca; Peel, Alan (March 2008). "Our Peculiar Motion Away from the Local Void".The Astrophysical Journal.676 (1):184–205.arXiv:0705.4139.Bibcode:2008ApJ...676..184T.doi:10.1086/527428.S2CID 14738309.
  3. ^abTully, R. Brent (May 2008). "The Local Void is Really Empty".Proceedings of the International Astronomical Union.244:146–151.arXiv:0708.0864.Bibcode:2008IAUS..244..146T.doi:10.1017/S1743921307013932.S2CID 119643726.
  4. ^"Milky Way amidst a 'Council of Giants'".Science Daily. 11 March 2014.
  5. ^Shaya, E. J.; Tully, R. B. (2013)."The formation of Local Group planes of galaxies".Monthly Notices of the Royal Astronomical Society.436 (3):2096–2119.arXiv:1307.4297.Bibcode:2013MNRAS.436.2096S.doi:10.1093/mnras/stt1714.
  6. ^abTully, R. Brent (2008). "The Local Velocity Anomaly".Galaxies in the Local Volume. Astrophysics and Space Science Proceedings. Vol. 5. pp. 3–12.arXiv:0708.2449.Bibcode:2008ASSP....5....3T.doi:10.1007/978-1-4020-6933-8_1.ISBN 978-1-4020-6932-1.
  7. ^Tully, R. Brent; Fisher, J. Richard (1987).Atlas of Nearby Galaxies.Bibcode:1987ang..book.....T.
  8. ^abMüller, Oliver; Scalera, Roberto; Binggeli, Bruno; Jerjen, Helmut (June 2017)."The M 101 group complex: new dwarf galaxy candidates and spatial structure".Astronomy & Astrophysics.602: A119.arXiv:1701.03681.Bibcode:2017A&A...602A.119M.doi:10.1051/0004-6361/201730434.ISSN 0004-6361.
  9. ^Tully, R. Brent; Verheijen, Marc A. W.; Pierce, Michael J.; Huang, Jia-Sheng; Wainscoat, Richard J. (December 1996)."The Ursa Major Cluster of Galaxies.I.Cluster Definition and Photometric Data".The Astronomical Journal.112: 2471.arXiv:astro-ph/9608124.Bibcode:1996AJ....112.2471T.doi:10.1086/118196.ISSN 0004-6256.
  10. ^Hartwick, F. D. A. (May 2000)."The Structure of the Outer Halo of the Galaxy and its Relationship to Nearby Large-Scale Structure".The Astronomical Journal.119 (5):2248–2253.arXiv:astro-ph/9912083.Bibcode:2000AJ....119.2248H.doi:10.1086/301332.
  11. ^Burstein, D. (2000). "Elliptical galaxies dynamics: The issues pertaining to galaxy formation". In F. Hammer; T. X. Thuan; V. Cayatte; B. Guiderdoni; J. T. Thanh Van (eds.).Building Galaxies: From the Primordial Universe to the Present: Proceedings of the XIXth Rencontres de Moriond held at Les Arcs, March 13-20, 1999. World Scientific Publishing. p. 85.arXiv:astro-ph/9908355.Bibcode:2000bgfp.conf...85B.ISBN 981-02-4411-8.
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