Galaxy_filament

Galaxy filament

Galaxy filament

Largest structures in the universe, made of galaxies


In cosmology, galaxy filaments are the largest known structures in the universe, consisting of walls of galactic superclusters. These massive, thread-like formations can commonly reach 50/h to 80/h Megaparsecs (160 to 260 megalight-years)—with the largest found to date being the Hercules-Corona Borealis Great Wall at around 3 gigaparsecs (9.8 Gly) in length—and form the boundaries between voids.[1] Due to the accelerating expansion of the universe, the individual clusters of gravitationally bound galaxies that make up galaxy filaments are moving away from each other at an accelerated rate; in the far future they will dissolve.[2]

Galaxy filaments, walls and voids form web-like structures. Computer simulation.

Galaxy filaments form the cosmic web and define the overall structure of the observable universe.[3][4][5]

Discovery

Discovery of structures larger than superclusters began in the late 1980s. In 1987, astronomer R. Brent Tully of the University of Hawaii's Institute of Astronomy identified what he called the Pisces–Cetus Supercluster Complex. The CfA2 Great Wall was discovered in 1989,[6] followed by the Sloan Great Wall in 2003.[7]

In January 2013, researchers led by Roger Clowes of the University of Central Lancashire announced the discovery of a large quasar group, the Huge-LQG, which dwarfs previously discovered galaxy filaments in size.[8] In November 2013, using gamma-ray bursts as reference points, astronomers discovered the Hercules–Corona Borealis Great Wall, an extremely large filament measuring more than 10 billion light-years across.[9][10][11]

Filaments

The filament subtype of filaments have roughly similar major and minor axes in cross-section, along the lengthwise axis.

More information Filament, Date ...
  • A short filament was proposed by Adi Zitrin and Noah Brosch—detected by identifying an alignment of star-forming galaxies—in the neighborhood of the Milky Way and the Local Group.[20] The proposal of this filament, and of a similar but shorter filament, were the result of a study by McQuinn et al. (2014) based on distance measurements using the TRGB method.[21]

Galaxy walls

The galaxy wall subtype of filaments have a significantly greater major axis than minor axis in cross-section, along the lengthwise axis.

More information Wall, Date ...
  • A "Centaurus Great Wall" (or "Fornax Great Wall" or "Virgo Great Wall") has been proposed, which would include the Fornax Wall as a portion of it (visually created by the Zone of Avoidance) along with the Centaurus Supercluster and the Virgo Supercluster, also known as the Local Supercluster, within which the Milky Way galaxy is located (implying this to be the Local Great Wall).[24][25]
  • A wall was proposed to be the physical embodiment of the Great Attractor, with the Norma Cluster as part of it. It is sometimes referred to as the Great Attractor Wall or Norma Wall.[26] This suggestion was superseded by the proposal of a supercluster, Laniakea, that would encompass the Great Attractor, Virgo Supercluster, Hydra–Centaurus Superclusters.[27]
  • A wall was proposed in 2000 to lie at z=1.47 in the vicinity of radio galaxy B3 0003+387.[28]
  • A wall was proposed in 2000 to lie at z=0.559 in the northern Hubble Deep Field (HDF North).[29][30]

Map of nearest galaxy walls

The Universe within 500 million light years, showing the nearest galaxy walls

Large Quasar Groups

Large quasar groups (LQGs) are some of the largest structures known.[31] They are theorized to be protohyperclusters/proto-supercluster-complexes/galaxy filament precursors.[32]

More information LQG, Date ...

Supercluster complex

Pisces–Cetus Supercluster Complex

Maps of large-scale distribution

See also


References

  1. Bharadwaj, Somnath; Bhavsar, Suketu; Sheth, Jatush V (2004). "The Size of the Longest Filaments in the Universe". Astrophys J. 606 (1): 25–31. arXiv:astro-ph/0311342. Bibcode:2004ApJ...606...25B. doi:10.1086/382140. S2CID 10473973.
  2. Siegel, Ethan. "Our Home Supercluster, Laniakea, Is Dissolving Before Our Eyes". Forbes. Retrieved 2023-11-13.
  3. "Cosmic Web". NASA Universe Exploration. Archived from the original on 2023-03-27. Retrieved 2023-06-06.
  4. Boris V. Komberg, Andrey V. Kravtsov, Vladimir N. Lukash; "The search and investigation of the Large Groups of Quasars" arXiv:astro-ph/9602090; Bibcode:1996astro.ph..2090K;
  5. R. G. Clowes; "Large Quasar Groups – A Short Review"; The New Era of Wide Field Astronomy, ASP Conference Series, vol. 232.; 2001; Astronomical Society of the Pacific; ISBN 1-58381-065-X; Bibcode:2001ASPC..232..108C
  6. Huchra, John P.; Geller, Margaret J. (17 November 1989). "M. J. Geller & J. P. Huchra, Science 246, 897 (1989)". Science. 246 (4932): 897–903. doi:10.1126/science.246.4932.897. PMID 17812575. S2CID 31328798. Archived from the original on 2008-06-21. Retrieved 2009-09-18.
  7. Sky and Telescope, "Refining the Cosmic Recipe" Archived 2012-03-09 at the Wayback Machine, 14 November 2003
  8. Wall, Mike (2013-01-11). "Largest structure in universe discovered". Fox News. Archived from the original on 2013-01-12. Retrieved 2013-01-12.
  9. Horvath, Istvan; Hakkila, Jon; Bagoly, Zsolt (2014). "Possible structure in the GRB sky distribution at redshift two". Astronomy & Astrophysics. 561: id.L12. arXiv:1401.0533. Bibcode:2014A&A...561L..12H. doi:10.1051/0004-6361/201323020. S2CID 24224684.
  10. Horvath I., Hakkila J., and Bagoly Z.; Hakkila, J.; Bagoly, Z. (2013). "The largest structure of the Universe, defined by Gamma-Ray Bursts". 7th Huntsville Gamma-Ray Burst Symposium, GRB 2013: Paper 33 in EConf Proceedings C1304143. 1311: 1104. arXiv:1311.1104. Bibcode:2013arXiv1311.1104H.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  11. Klotz, Irene (2013-11-19). "Universe's Largest Structure is a Cosmic Conundrum". discovery. Archived from the original on 2013-11-30. Retrieved 2013-11-22.
  12. 'Astronomy and Astrophysics' (ISSN 0004-6361), vol. 138, no. 1, Sept. 1984, pp. 85–92. Research supported by Cornell University "The Coma/A 1367 filament of galaxies" 09/1984 Bibcode:1984A&A...138...85F
  13. 'Astrophysical Journal', Part 1 (ISSN 0004-637X), vol. 299, Dec. 1, 1985, pp. 5–14. "A possible 300 megaparsec filament of clusters of galaxies in Perseus-Pegasus" 12/1985 Bibcode:1985ApJ...299....5B
  14. The Astrophysical Journal Supplement Series, volume 121, issue 2, pp. 445–472. "Photometric Properties of Kiso Ultraviolet-Excess Galaxies in the Lynx-Ursa Major Region" 04/1999 Bibcode:1999ApJS..121..445T
  15. Palunas, Povilas; Teplitz, Harry I.; Francis, Paul J.; Williger, Gerard M.; Woodgate, Bruce E. (2004). "The Distribution of Lyα‐Emitting Galaxies at z = 2.38". The Astrophysical Journal. 602 (2): 545–554. arXiv:astro-ph/0311279. Bibcode:2004ApJ...602..545P. doi:10.1086/381145. S2CID 990891.
  16. Francis, Paul J.; Palunas, Povilas; Teplitz, Harry I.; Williger, Gerard M.; Woodgate, Bruce E. (2004). "The Distribution of Lyα‐emitting Galaxies at z =2.38. II. Spectroscopy". The Astrophysical Journal. 614 (1): 75–83. arXiv:astro-ph/0406413. Bibcode:2004ApJ...614...75F. doi:10.1086/423417. S2CID 118037575.
  17. Relativistic Astrophysics Legacy and Cosmology - Einstein's, ESO Astrophysics Symposia, Volume . ISBN 978-3-540-74712-3. Springer-Verlag Berlin Heidelberg, 2008, p. 358 "Ultraviolet-Bright, High-Redshift ULIRGS" 00/2008 Bibcode:2008ralc.conf..358W
  18. Zitrin, A.; Brosch, N. (2008). "The NGC 672 and 784 galaxy groups: evidence for galaxy formation and growth along a nearby dark matter filament". Monthly Notices of the Royal Astronomical Society. 390 (1): 408–420. arXiv:0808.1789. Bibcode:2008MNRAS.390..408Z. doi:10.1111/j.1365-2966.2008.13786.x. S2CID 16296617.
  19. McQuinn, K.B.W.; et al. (2014). "Distance Determinations to SHIELD Galaxies from Hubble Space Telescope Imaging". The Astrophysical Journal. 785 (1): 3. arXiv:1402.3723. Bibcode:2014ApJ...785....3M. doi:10.1088/0004-637x/785/1/3. S2CID 118465292.
  20. Chin. J. Astron. Astrophys. Vol. 6 (2006), No. 1, 35–42 "Super-Large-Scale Structures in the Sloan Digital Sky Survey" (PDF). Archived (PDF) from the original on 2013-06-10. Retrieved 2008-08-02.
  21. Scientific American, vol. 280, no. 6, pp. 30–37 "Mapping the Universe" (PDF). Archived from the original (PDF) on 2008-07-04. (1.43 MB) 06/1999 Bibcode:1999SciAm.280f..30L
  22. Unveiling large-scale structures behind the Milky Way. Astronomical Society of the Pacific Conference Series, vol. 67; Proceedings of a workshop at the Observatoire de Paris-Meudon; 18–21 January 1994; San Francisco, California: Astronomical Society of the Pacific (ASP); c1994; edited by Chantal Balkowski and R. C. Kraan-Korteweg, p.21; Visualization of Nearby Large-Scale Structures Archived 2015-11-27 at the Wayback Machine; Fairall, A. P.; Paverd, W. R.; & Ashley, R. P.; 1994 ASPC...67...21F
  23. Astrophysics and Space Science, volume 230, issue 1–2, pp. 225–235 "Large-Scale Structures in the Distribution of Galaxies" 08/1995 Bibcode:1995Ap&SS.230..225F
  24. World Science, Wall of galaxies tugs on ours, astronomers find Archived 2007-10-28 at the Wayback Machine April 19, 2006
  25. Tully, R. Brent; Courtois, Hélène; Hoffman, Yehuda; Pomarède, Daniel (2 September 2014). "The Laniakea supercluster of galaxies". Nature. 513 (7516) (published 4 September 2014): 71–73. arXiv:1409.0880. Bibcode:2014Natur.513...71T. doi:10.1038/nature13674. PMID 25186900. S2CID 205240232.
  26. The Astronomical Journal, volume 120, issue 5, pp. 2331–2337. "B3 0003+387: AGN-Marked Large-Scale Structure at Redshift 1.47?" 11/2000 Bibcode:2000AJ....120.2331T doi:10.1086/316827
  27. Vanden Berk, Daniel E.; Stoughton, Chris; Crotts, Arlin P. S.; Tytler, David; Kirkman, David (2000). "QSO[CLC]s[/CLC] and Absorption-Line Systems surrounding the Hubble Deep Field". The Astronomical Journal. 119 (6): 2571–2582. arXiv:astro-ph/0003203. Bibcode:2000AJ....119.2571V. doi:10.1086/301404. S2CID 117882449.
  28. Clowes, Roger G.; Harris, Kathryn A.; Raghunathan, Srinivasan; Campusano, Luis E.; Soechting, Ilona K.; Graham, Matthew J.; "A structure in the early universe at z ~ 1.3 that exceeds the homogeneity scale of the R-W concordance cosmology"; arXiv:1211.6256; Bibcode:2012arXiv1211.6256C; doi:10.1093/mnras/sts497; Monthly Notices of the Royal Astronomical Society, 11 January 2013

Further reading


Share this article:

This article uses material from the Wikipedia article Galaxy_filament, and is written by contributors. Text is available under a CC BY-SA 4.0 International License; additional terms may apply. Images, videos and audio are available under their respective licenses.