![Galaxy filament](https://www.english.nina.az/wikipedia/image/aHR0cHM6Ly91cGxvYWQud2lraW1lZGlhLm9yZy93aWtpcGVkaWEvY29tbW9ucy90aHVtYi82LzZkL0xhcmdlLXNjYWxlX3N0cnVjdHVyZV9vZl9saWdodF9kaXN0cmlidXRpb25faW5fdGhlX3VuaXZlcnNlLmpwZy8xNjAwcHgtTGFyZ2Utc2NhbGVfc3RydWN0dXJlX29mX2xpZ2h0X2Rpc3RyaWJ1dGlvbl9pbl90aGVfdW5pdmVyc2UuanBn.jpg )
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 to 80 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. 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.
![image](https://www.english.nina.az/wikipedia/image/aHR0cHM6Ly93d3cuZW5nbGlzaC5uaW5hLmF6L3dpa2lwZWRpYS9pbWFnZS9hSFIwY0hNNkx5OTFjR3h2WVdRdWQybHJhVzFsWkdsaExtOXlaeTkzYVd0cGNHVmthV0V2WTI5dGJXOXVjeTkwYUhWdFlpODJMelprTDB4aGNtZGxMWE5qWVd4bFgzTjBjblZqZEhWeVpWOXZabDlzYVdkb2RGOWthWE4wY21saWRYUnBiMjVmYVc1ZmRHaGxYM1Z1YVhabGNuTmxMbXB3Wnk4eU5qQndlQzFNWVhKblpTMXpZMkZzWlY5emRISjFZM1IxY21WZmIyWmZiR2xuYUhSZlpHbHpkSEpwWW5WMGFXOXVYMmx1WDNSb1pWOTFibWwyWlhKelpTNXFjR2M9LmpwZw==.jpg)
Galaxy filaments form the cosmic web and define the overall structure of the observable universe.
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, followed by the Sloan Great Wall in 2003.
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. 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.
Filaments
The filament subtype of filaments have roughly similar major and minor axes in cross-section, along the lengthwise axis.
Filament | Date | Mean distance | Dimension | Notes |
---|---|---|---|---|
Coma Filament | The Coma Supercluster lies within the Coma Filament. It forms part of the CfA2 Great Wall. | |||
Perseus–Pegasus Filament | 1985 | Connected to the Pisces–Cetus Supercluster, with the Perseus–Pisces Supercluster being a member of the filament. | ||
Ursa Major Filament | Connected to the CfA Homunculus, a portion of the filament forms a portion of the "leg" of the Homunculus. | |||
Lynx–Ursa Major Filament (LUM Filament) | 1999 | from 2000 km/s to 8000 km/s in redshift space | Connected to and separate from the Lynx–Ursa Major Supercluster. | |
z=2.38 filament around protocluster ClG J2143-4423 | 2004 | z=2.38 | 110 Mpc | A filament the length of the Great Wall was discovered in 2004. As of 2008, it was still the largest structure beyond redshift 2. |
- 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. 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.
Galaxy walls
The galaxy wall subtype of filaments have a significantly greater major axis than minor axis in cross-section, along the lengthwise axis.
Wall | Date | Mean distance | Dimension | Notes |
---|---|---|---|---|
CfA2 Great Wall (Coma Wall, Great Wall, Northern Great Wall, Great Northern Wall, CfA Great Wall) | 1989 | z=0.03058 | 251 Mpc long: 750 Mly long 250 Mly wide 20 Mly thick | This was the first super-large large-scale structure or pseudo-structure in the universe to be discovered. The CfA Homunculus lies at the heart of the Great Wall, and the Coma Supercluster forms most of the homunculus structure. The Coma Cluster lies at the core. |
Sloan Great Wall (SDSS Great Wall) | 2003 | z=0.07804 | 433 Mpc long | This was the largest known galaxy filament to be discovered, until it was eclipsed by the Hercules–Corona Borealis Great Wall found ten years later. |
Sculptor Wall (Southern Great Wall, Great Southern Wall, Southern Wall) | 8000 km/s long 5000 km/s wide 1000 km/s deep (in redshift space dimensions) | The Sculptor Wall is "parallel" to the Fornax Wall and "perpendicular" to the Grus Wall. | ||
Grus Wall | The Grus Wall is "perpendicular" to the Fornax and Sculptor Walls. | |||
Fornax Wall | The Fornax Cluster is part of this wall. The wall is "parallel" to the Sculptor Wall and "perpendicular" to the Grus Wall. | |||
Hercules–Corona Borealis Great Wall | 2013 | z≈2 | 3 Gpc long, 150 000 km/s deep (in redshift space) | The largest known structure in the universe. This is also the first time since 1991 that a galaxy filament/great wall held the record as the largest known structure in the universe. |
- 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).
- 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 or . This suggestion was superseded by the proposal of a supercluster, Laniakea, that would encompass the Great Attractor, Virgo Supercluster, Hydra–Centaurus Superclusters.
- A wall was proposed in 2000 to lie at z=1.47 in the vicinity of radio galaxy .
- A wall was proposed in 2000 to lie at z=0.559 in the northern Hubble Deep Field (HDF North).
Map of nearest galaxy walls
![image](https://www.english.nina.az/wikipedia/image/aHR0cHM6Ly93d3cuZW5nbGlzaC5uaW5hLmF6L3dpa2lwZWRpYS9pbWFnZS9hSFIwY0hNNkx5OTFjR3h2WVdRdWQybHJhVzFsWkdsaExtOXlaeTkzYVd0cGNHVmthV0V2WTI5dGJXOXVjeTlrTDJRNEwwNWxZWEp6WXk1bmFXWT0uZ2lm.gif)
Large Quasar Groups
Large quasar groups (LQGs) are some of the largest structures known. They are theorized to be protohyperclusters/proto-supercluster-complexes/galaxy filament precursors.
LQG | Date | Mean distance | Dimension | Notes |
---|---|---|---|---|
Clowes–Campusano LQG (U1.28, CCLQG) | 1991 | z=1.28 |
| It was the largest known structure in the universe from 1991 to 2011, until U1.11's discovery. |
U1.11 | 2011 | z=1.11 |
| Was the largest known structure in the universe for a few months, until Huge-LQG's discovery. |
Huge-LQG | 2012 | z=1.27 |
| It was the largest structure known in the universe, until the discovery of the Hercules–Corona Borealis Great Wall found one year later. |
Supercluster complex
Pisces–Cetus Supercluster Complex
Maps of large-scale distribution
- The universe within 1 billion light-years (307 Mpc) of Earth, showing local superclusters forming filaments and voids
- Map of nearest walls, voids and superclusters
- 2dF survey map, containing the SDSS Great Wall
- 2MASS XSC infrared sky map
- A mosaic MeerKAT image of the Galactic Center at 20 cm with a 4 resolution.
See also
- List of largest cosmic structures
- Galaxy
- Galaxy cluster
- Galaxy supercluster
- Illustris project
- Large-scale structure
- List of galaxies
- List of galaxy groups and clusters
- Void (astronomy)
- Infrared cirrus
References
- 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.
- Siegel, Ethan. "Our Home Supercluster, Laniakea, Is Dissolving Before Our Eyes". Forbes. Retrieved 2023-11-13.
- "Cosmic Web". NASA Universe Exploration. Archived from the original on 2023-03-27. Retrieved 2023-06-06.
- Komberg, B. V.; Kravtsov, A. V.; Lukash, V. N. (October 1996). "The search for and investigation of large quasar groups". Monthly Notices of the Royal Astronomical Society. 282 (3): 713–722. arXiv:astro-ph/9602090. Bibcode:1996MNRAS.282..713K. doi:10.1093/mnras/282.3.713. ISSN 0035-8711.
- Clowes, R. G. (2001). "Large Quasar Groups - A Short Review". Astronomical Society of the Pacific. 232: 108. Bibcode:2001ASPC..232..108C. ISBN 1-58381-065-X.
- 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.
- Sky and Telescope, "Refining the Cosmic Recipe" Archived 2012-03-09 at the Wayback Machine, 14 November 2003
- Wall, Mike (2013-01-11). "Largest structure in universe discovered". Fox News. Archived from the original on 2013-01-12. Retrieved 2013-01-12.
- 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.
- 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}}
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- Fontanelli, P. (1983). "Clustering in the Universe: A filament of galaxies in the Coma/A1367 supercluster". Astronomy and Astrophysics. 138: 85–92. Bibcode:1984A&A...138...85F. ISSN 0004-6361.
- Gavazzi, Giuseppe; Catinella, Barbara; Carrasco, Luis; et al. (May 1998). "The Star Formation Properties of Disk Galaxies: Hα Imaging of Galaxies in the Coma Supercluster". The Astronomical Journal. 115 (5): 1745–1777. arXiv:astro-ph/9801279. Bibcode:1998AJ....115.1745G. doi:10.1086/300314.
- Batuski, D. J.; Burns, J. O. (December 1985). "A possible 300 megaparsec filament of clusters of galaxies in Perseus-Pegasus". The Astrophysical Journal. 299: 5. Bibcode:1985ApJ...299....5B. doi:10.1086/163677. ISSN 0004-637X.
- Takeuchi, Tsutomu T.; Tomita, Akihiko; Nakanishi, Kouichiro; Ishii, Takako T.; Iwata, Ikuru; Saitō, Mamoru (April 1999). "Photometric Properties of Kiso Ultraviolet-Excess Galaxies in the Lynx–Ursa Major Region". The Astrophysical Journal Supplement Series. 121 (2): 445–472. arXiv:astro-ph/9810161. Bibcode:1999ApJS..121..445T. doi:10.1086/313203. ISSN 0067-0049.
- NASA, GIANT GALAXY STRING DEFIES MODELS OF HOW UNIVERSE EVOLVED Archived 2008-08-06 at the Wayback Machine, January 7, 2004
- 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.
- 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.
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- FermiLab, "Astronomers Find Wall of Galaxies Traversing the Hubble Deep Field", DARPA, Monday, January 24, 2000
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- Yusef-Zadeh, F.; Arendt, R. G.; Wardle, M.; Heywood, I. (1 June 2023). "The Population of the Galactic Center Filaments: Position Angle Distribution Reveals a Degree-scale Collimated Outflow from Sgr A* along the Galactic Plane". The Astrophysical Journal Letters. 949 (2): L31. arXiv:2306.01071. Bibcode:2023ApJ...949L..31Y. doi:10.3847/2041-8213/acd54b. ISSN 2041-8205. S2CID 259046030.
Further reading
- Pimbblet, Kevin A. (2005). "Pulling Out Threads from the Cosmic Tapestry: Defining Filaments of Galaxies". Publications of the Astronomical Society of Australia. 22 (2): 136–143. arXiv:astro-ph/0503286. Bibcode:2005PASA...22..136P. doi:10.1071/AS05006. ISSN 1323-3580.
External links
- Pictures of the filamentary network
- The Universe Within One Billion Light Years with List of Nearby Superclusters (from the Atlas of the Universe):
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 to 80 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 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 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 DiscoveryDiscovery 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 followed by the Sloan Great Wall in 2003 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 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 FilamentsThe filament subtype of filaments have roughly similar major and minor axes in cross section along the lengthwise axis Filaments of Galaxies Filament Date Mean distance Dimension NotesComa Filament The Coma Supercluster lies within the Coma Filament It forms part of the CfA2 Great Wall Perseus Pegasus Filament 1985 Connected to the Pisces Cetus Supercluster with the Perseus Pisces Supercluster being a member of the filament Ursa Major Filament Connected to the CfA Homunculus a portion of the filament forms a portion of the leg of the Homunculus Lynx Ursa Major Filament LUM Filament 1999 from 2000 km s to 8000 km s in redshift space Connected to and separate from the Lynx Ursa Major Supercluster z 2 38 filament around protocluster ClG J2143 4423 2004 z 2 38 110 Mpc A filament the length of the Great Wall was discovered in 2004 As of 2008 it was still the largest structure beyond redshift 2 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 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 Galaxy walls The galaxy wall subtype of filaments have a significantly greater major axis than minor axis in cross section along the lengthwise axis Walls of Galaxies Wall Date Mean distance Dimension NotesCfA2 Great Wall Coma Wall Great Wall Northern Great Wall Great Northern Wall CfA Great Wall 1989 z 0 03058 251 Mpc long 750 Mly long 250 Mly wide 20 Mly thick This was the first super large large scale structure or pseudo structure in the universe to be discovered The CfA Homunculus lies at the heart of the Great Wall and the Coma Supercluster forms most of the homunculus structure The Coma Cluster lies at the core Sloan Great Wall SDSS Great Wall 2003 z 0 07804 433 Mpc long This was the largest known galaxy filament to be discovered until it was eclipsed by the Hercules Corona Borealis Great Wall found ten years later Sculptor Wall Southern Great Wall Great Southern Wall Southern Wall 8000 km s long 5000 km s wide 1000 km s deep in redshift space dimensions The Sculptor Wall is parallel to the Fornax Wall and perpendicular to the Grus Wall Grus Wall The Grus Wall is perpendicular to the Fornax and Sculptor Walls Fornax Wall The Fornax Cluster is part of this wall The wall is parallel to the Sculptor Wall and perpendicular to the Grus Wall Hercules Corona Borealis Great Wall 2013 z 2 3 Gpc long 150 000 km s deep in redshift space The largest known structure in the universe This is also the first time since 1991 that a galaxy filament great wall held the record as the largest known structure in the universe 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 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 or This suggestion was superseded by the proposal of a supercluster Laniakea that would encompass the Great Attractor Virgo Supercluster Hydra Centaurus Superclusters A wall was proposed in 2000 to lie at z 1 47 in the vicinity of radio galaxy A wall was proposed in 2000 to lie at z 0 559 in the northern Hubble Deep Field HDF North Map of nearest galaxy walls The Universe within 500 million light years showing the nearest galaxy wallsLarge Quasar Groups Large quasar groups LQGs are some of the largest structures known They are theorized to be protohyperclusters proto supercluster complexes galaxy filament precursors Large Quasar Groups LQG Date Mean distance Dimension NotesClowes Campusano LQG U1 28 CCLQG 1991 z 1 28 longest dimension 630 Mpc It was the largest known structure in the universe from 1991 to 2011 until U1 11 s discovery U1 11 2011 z 1 11 longest dimension 780 Mpc Was the largest known structure in the universe for a few months until Huge LQG s discovery Huge LQG 2012 z 1 27 characteristic size 500 Mpc longest dimension 1 24 Gpc It was the largest structure known in the universe until the discovery of the Hercules Corona Borealis Great Wall found one year later Supercluster complex Pisces Cetus Supercluster ComplexMaps of large scale distributionThe universe within 1 billion light years 307 Mpc of Earth showing local superclusters forming filaments and voids Map of nearest walls voids and superclusters 2dF survey map containing the SDSS Great Wall 2MASS XSC infrared sky map A mosaic MeerKAT image of the Galactic Center at 20 cm with a 4resolution See alsoList of largest cosmic structures Galaxy Galaxy cluster Galaxy supercluster Illustris project Large scale structure List of galaxies List of galaxy groups and clusters Void astronomy Infrared cirrusReferencesBharadwaj 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 Siegel Ethan Our Home Supercluster Laniakea Is Dissolving Before Our Eyes Forbes Retrieved 2023 11 13 Cosmic Web NASA Universe Exploration Archived from the original on 2023 03 27 Retrieved 2023 06 06 Komberg B V Kravtsov A V Lukash V N October 1996 The search for and investigation of large quasar groups Monthly Notices of the Royal Astronomical Society 282 3 713 722 arXiv astro ph 9602090 Bibcode 1996MNRAS 282 713K doi 10 1093 mnras 282 3 713 ISSN 0035 8711 Clowes R G 2001 Large Quasar Groups A Short Review Astronomical Society of the Pacific 232 108 Bibcode 2001ASPC 232 108C ISBN 1 58381 065 X Huchra John P Geller Margaret J 17 November 1989 M J Geller amp 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 Sky and Telescope Refining the Cosmic Recipe Archived 2012 03 09 at the Wayback Machine 14 November 2003 Wall Mike 2013 01 11 Largest structure in universe discovered Fox News Archived from the original on 2013 01 12 Retrieved 2013 01 12 Horvath Istvan Hakkila Jon Bagoly Zsolt 2014 Possible structure in the GRB sky distribution at redshift two Astronomy amp Astrophysics 561 id L12 arXiv 1401 0533 Bibcode 2014A amp A 561L 12H doi 10 1051 0004 6361 201323020 S2CID 24224684 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 a href wiki Template Cite journal title Template Cite journal cite journal a CS1 maint multiple names authors list link 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 Fontanelli P 1983 Clustering in the Universe A filament of galaxies in the Coma A1367 supercluster Astronomy and Astrophysics 138 85 92 Bibcode 1984A amp A 138 85F ISSN 0004 6361 Gavazzi Giuseppe Catinella Barbara Carrasco Luis et al May 1998 The Star Formation Properties of Disk Galaxies Ha Imaging 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astronomers find Archived 2007 10 28 at the Wayback Machine April 19 2006 Tully R Brent Courtois Helene Hoffman Yehuda Pomarede 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 Thompson D Aftreth O Soifer B T November 2000 B3 0003 387 AGN Marked Large Scale Structure at Redshift 1 47 The Astronomical Journal 120 5 2331 2337 arXiv astro ph 0008030 Bibcode 2000AJ 120 2331T doi 10 1086 316827 FermiLab Astronomers Find Wall of Galaxies Traversing the Hubble Deep Field DARPA Monday January 24 2000 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 Biggest structure in universe Large quasar group is 4 billion light years across ScienceDaily Retrieved 2023 09 16 Clowes Roger G Harris Kathryn A Raghunathan Srinivasan Campusano Luis E Sochting Ilona K Graham Matthew J March 2013 A structure in the early Universe at z 1 3 that exceeds the homogeneity scale of the R W concordance cosmology Monthly Notices of the Royal Astronomical Society 429 4 2910 2916 arXiv 1211 6256 doi 10 1093 mnras sts497 ISSN 1365 2966 Yusef Zadeh F Arendt R G Wardle M Heywood I 1 June 2023 The Population of the Galactic Center Filaments Position Angle Distribution Reveals a Degree scale Collimated Outflow from Sgr A along the Galactic Plane The Astrophysical Journal Letters 949 2 L31 arXiv 2306 01071 Bibcode 2023ApJ 949L 31Y doi 10 3847 2041 8213 acd54b ISSN 2041 8205 S2CID 259046030 Further readingPimbblet Kevin A 2005 Pulling Out Threads from the Cosmic Tapestry Defining Filaments of Galaxies Publications of the Astronomical Society of Australia 22 2 136 143 arXiv astro ph 0503286 Bibcode 2005PASA 22 136P doi 10 1071 AS05006 ISSN 1323 3580 External linksPictures of the filamentary network The Universe Within One Billion Light Years with List of Nearby Superclusters from the Atlas of the Universe Portals StarsSpaceflightOuter spaceSolar SystemScience