Cosmicflows-3: The South Pole Wall
Velocity and density field reconstructions of the volume of the universe within 0.05c derived from the Cosmicflows-3 catalog of galaxy distances has revealed the presence of a filamentary structure extending across ∼0.11c. The structure, at a characteristic redshift of 12,000 km s−1, has a density p...
Gespeichert in:
Veröffentlicht in: | The Astrophysical journal 2020-07, Vol.897 (2), p.133 |
---|---|
Hauptverfasser: | , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext bestellen |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | 2 |
container_start_page | 133 |
container_title | The Astrophysical journal |
container_volume | 897 |
creator | Pomarède, Daniel Tully, R. Brent Graziani, Romain Courtois, Hélène M. Hoffman, Yehuda Lezmy, Jérémy |
description | Velocity and density field reconstructions of the volume of the universe within 0.05c derived from the Cosmicflows-3 catalog of galaxy distances has revealed the presence of a filamentary structure extending across ∼0.11c. The structure, at a characteristic redshift of 12,000 km s−1, has a density peak coincident with the celestial South Pole. This structure, the largest contiguous feature in the local volume and comparable to the Sloan Great Wall at half the distance, is given the name the South Pole Wall. |
doi_str_mv | 10.3847/1538-4357/ab9952 |
format | Article |
fullrecord | <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_proquest_journals_2423576218</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2423576218</sourcerecordid><originalsourceid>FETCH-LOGICAL-c384t-1976e99348c0118a8b1c0020c91128bf92de8d75f8c7c9b03f8ba6a9a12d844c3</originalsourceid><addsrcrecordid>eNp1kEFLw0AQhRdRsFbvHoOeBGNndjfJjrcSqhUKClb0tmy2G5qSujXbKv57EyL15GmY4XuPN4-xc4QboWQ2wkSoWIokG5mCKOEHbLA_HbIBAMg4FdnbMTsJYdWtnGjALnIf1pUta_8VYnEbzZcueva77TJ68rWLXk1dn7Kj0tTBnf3OIXu5m8zzaTx7vH_Ix7PYtgG2MVKWOiIhlQVEZVSBFoCDJUSuipL4wqlFlpTKZpYKEKUqTGrIIF8oKa0Ysqved2lqvWmqtWm-tTeVno5nursBJ0iQ-Ce27GXPbhr_sXNhq1d-17y38TSXvH055ahaCnrKNj6ExpV7WwTdtaa7inRXke5bayXXvaTymz_Pf_EfzuBpMQ</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2423576218</pqid></control><display><type>article</type><title>Cosmicflows-3: The South Pole Wall</title><source>IOP Publishing Free Content</source><creator>Pomarède, Daniel ; Tully, R. Brent ; Graziani, Romain ; Courtois, Hélène M. ; Hoffman, Yehuda ; Lezmy, Jérémy</creator><creatorcontrib>Pomarède, Daniel ; Tully, R. Brent ; Graziani, Romain ; Courtois, Hélène M. ; Hoffman, Yehuda ; Lezmy, Jérémy</creatorcontrib><description>Velocity and density field reconstructions of the volume of the universe within 0.05c derived from the Cosmicflows-3 catalog of galaxy distances has revealed the presence of a filamentary structure extending across ∼0.11c. The structure, at a characteristic redshift of 12,000 km s−1, has a density peak coincident with the celestial South Pole. This structure, the largest contiguous feature in the local volume and comparable to the Sloan Great Wall at half the distance, is given the name the South Pole Wall.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/1538-4357/ab9952</identifier><language>eng</language><publisher>Philadelphia: The American Astronomical Society</publisher><subject>Astrophysics ; Cosmology ; Density ; Galaxies ; Large-scale structure of the universe ; Physics ; Red shift ; South Pole</subject><ispartof>The Astrophysical journal, 2020-07, Vol.897 (2), p.133</ispartof><rights>2020. The American Astronomical Society. All rights reserved.</rights><rights>Copyright IOP Publishing Jul 01, 2020</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c384t-1976e99348c0118a8b1c0020c91128bf92de8d75f8c7c9b03f8ba6a9a12d844c3</citedby><cites>FETCH-LOGICAL-c384t-1976e99348c0118a8b1c0020c91128bf92de8d75f8c7c9b03f8ba6a9a12d844c3</cites><orcidid>0000-0002-9291-1981 ; 0000-0003-0509-1776 ; 0000-0003-2038-0488</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4357/ab9952/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>230,314,777,781,882,27905,27906,38871,53848</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4357/ab9952$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttps://hal.science/hal-02905192$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Pomarède, Daniel</creatorcontrib><creatorcontrib>Tully, R. Brent</creatorcontrib><creatorcontrib>Graziani, Romain</creatorcontrib><creatorcontrib>Courtois, Hélène M.</creatorcontrib><creatorcontrib>Hoffman, Yehuda</creatorcontrib><creatorcontrib>Lezmy, Jérémy</creatorcontrib><title>Cosmicflows-3: The South Pole Wall</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>Velocity and density field reconstructions of the volume of the universe within 0.05c derived from the Cosmicflows-3 catalog of galaxy distances has revealed the presence of a filamentary structure extending across ∼0.11c. The structure, at a characteristic redshift of 12,000 km s−1, has a density peak coincident with the celestial South Pole. This structure, the largest contiguous feature in the local volume and comparable to the Sloan Great Wall at half the distance, is given the name the South Pole Wall.</description><subject>Astrophysics</subject><subject>Cosmology</subject><subject>Density</subject><subject>Galaxies</subject><subject>Large-scale structure of the universe</subject><subject>Physics</subject><subject>Red shift</subject><subject>South Pole</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNp1kEFLw0AQhRdRsFbvHoOeBGNndjfJjrcSqhUKClb0tmy2G5qSujXbKv57EyL15GmY4XuPN4-xc4QboWQ2wkSoWIokG5mCKOEHbLA_HbIBAMg4FdnbMTsJYdWtnGjALnIf1pUta_8VYnEbzZcueva77TJ68rWLXk1dn7Kj0tTBnf3OIXu5m8zzaTx7vH_Ix7PYtgG2MVKWOiIhlQVEZVSBFoCDJUSuipL4wqlFlpTKZpYKEKUqTGrIIF8oKa0Ysqved2lqvWmqtWm-tTeVno5nursBJ0iQ-Ce27GXPbhr_sXNhq1d-17y38TSXvH055ahaCnrKNj6ExpV7WwTdtaa7inRXke5bayXXvaTymz_Pf_EfzuBpMQ</recordid><startdate>20200701</startdate><enddate>20200701</enddate><creator>Pomarède, Daniel</creator><creator>Tully, R. Brent</creator><creator>Graziani, Romain</creator><creator>Courtois, Hélène M.</creator><creator>Hoffman, Yehuda</creator><creator>Lezmy, Jérémy</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><general>American Astronomical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0002-9291-1981</orcidid><orcidid>https://orcid.org/0000-0003-0509-1776</orcidid><orcidid>https://orcid.org/0000-0003-2038-0488</orcidid></search><sort><creationdate>20200701</creationdate><title>Cosmicflows-3: The South Pole Wall</title><author>Pomarède, Daniel ; Tully, R. Brent ; Graziani, Romain ; Courtois, Hélène M. ; Hoffman, Yehuda ; Lezmy, Jérémy</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c384t-1976e99348c0118a8b1c0020c91128bf92de8d75f8c7c9b03f8ba6a9a12d844c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Astrophysics</topic><topic>Cosmology</topic><topic>Density</topic><topic>Galaxies</topic><topic>Large-scale structure of the universe</topic><topic>Physics</topic><topic>Red shift</topic><topic>South Pole</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pomarède, Daniel</creatorcontrib><creatorcontrib>Tully, R. Brent</creatorcontrib><creatorcontrib>Graziani, Romain</creatorcontrib><creatorcontrib>Courtois, Hélène M.</creatorcontrib><creatorcontrib>Hoffman, Yehuda</creatorcontrib><creatorcontrib>Lezmy, Jérémy</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Pomarède, Daniel</au><au>Tully, R. Brent</au><au>Graziani, Romain</au><au>Courtois, Hélène M.</au><au>Hoffman, Yehuda</au><au>Lezmy, Jérémy</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Cosmicflows-3: The South Pole Wall</atitle><jtitle>The Astrophysical journal</jtitle><stitle>APJ</stitle><addtitle>Astrophys. J</addtitle><date>2020-07-01</date><risdate>2020</risdate><volume>897</volume><issue>2</issue><spage>133</spage><pages>133-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>Velocity and density field reconstructions of the volume of the universe within 0.05c derived from the Cosmicflows-3 catalog of galaxy distances has revealed the presence of a filamentary structure extending across ∼0.11c. The structure, at a characteristic redshift of 12,000 km s−1, has a density peak coincident with the celestial South Pole. This structure, the largest contiguous feature in the local volume and comparable to the Sloan Great Wall at half the distance, is given the name the South Pole Wall.</abstract><cop>Philadelphia</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4357/ab9952</doi><tpages>9</tpages><orcidid>https://orcid.org/0000-0002-9291-1981</orcidid><orcidid>https://orcid.org/0000-0003-0509-1776</orcidid><orcidid>https://orcid.org/0000-0003-2038-0488</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | ISSN: 0004-637X |
ispartof | The Astrophysical journal, 2020-07, Vol.897 (2), p.133 |
issn | 0004-637X 1538-4357 |
language | eng |
recordid | cdi_proquest_journals_2423576218 |
source | IOP Publishing Free Content |
subjects | Astrophysics Cosmology Density Galaxies Large-scale structure of the universe Physics Red shift South Pole |
title | Cosmicflows-3: The South Pole Wall |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-19T22%3A43%3A07IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Cosmicflows-3:%20The%20South%20Pole%20Wall&rft.jtitle=The%20Astrophysical%20journal&rft.au=Pomar%C3%A8de,%20Daniel&rft.date=2020-07-01&rft.volume=897&rft.issue=2&rft.spage=133&rft.pages=133-&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.3847/1538-4357/ab9952&rft_dat=%3Cproquest_O3W%3E2423576218%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2423576218&rft_id=info:pmid/&rfr_iscdi=true |