Radio Traces of Cosmic Shock Waves

Radio Traces of Cosmic Shock Waves

Colliding and fusing galaxy clusters should produce giant shock waves. The outlines of these waves have now been seen as radio-emitting structures.

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Science (American Association for the Advancement of Science) 2006-11, Vol.314 (5800), p.772-773
1. Verfasser: Enslin, Torsten A
Format: Artikel
Sprache:eng
Schlagworte:
Accretion
Astronomy
Cosmology
Galaxies
Galaxy clusters
Mach number
Magnetic fields
Particle acceleration
Particle energy
Perspectives
Radio telescopes
Relativistic particles
Shock waves
Stars & galaxies
Thermal shock
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 773
container_issue 5800
container_start_page 772
container_title Science (American Association for the Advancement of Science)
container_volume 314
creator Enslin, Torsten A
description Colliding and fusing galaxy clusters should produce giant shock waves. The outlines of these waves have now been seen as radio-emitting structures.
doi_str_mv 10.1126/science.1133949
format Article
fullrecord <record><control><sourceid>jstor_proqu</sourceid><recordid>TN_cdi_proquest_miscellaneous_36184525</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><jstor_id>20031678</jstor_id><sourcerecordid>20031678</sourcerecordid><originalsourceid>FETCH-LOGICAL-c352t-d22213497611f82806f2b05e556a1c3aeefe9a9d7ad07694daab777757b24a183</originalsourceid><addsrcrecordid>eNqFkEtLAzEQgIMoWKtnT8LSg7e1mWTzOkrxBQVBKx7DbDaLW9umJlvBf2-kiwcvzmUY5pth5iPkHOgVAJPT5Dq_cT4XnJvKHJARUCNKwyg_JCNKuSw1VeKYnKS0pDT3DB-RyRM2XSgWEZ1PRWiLWUjrzhXPb8G9F6_46dMpOWpxlfzZkMfk5fZmMbsv5493D7Preem4YH3ZMMaAV0ZJgFYzTWXLaiq8EBLBcfS-9QZNo7ChSpqqQaxVDqFqViFoPiaX-73bGD52PvV23SXnVyvc-LBLlkvQlWDiXxAM15lTGZz8AZdhFzf5CZtPlUxJxjM03UMuhpSib-02dmuMXxao_TFrB7N2MJsnLvYTy9SH-Iuz7Bik0vwbK7Rziw</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>213627623</pqid></control><display><type>article</type><title>Radio Traces of Cosmic Shock Waves</title><source>American Association for the Advancement of Science</source><source>JSTOR</source><creator>Enslin, Torsten A</creator><creatorcontrib>Enslin, Torsten A</creatorcontrib><description>Colliding and fusing galaxy clusters should produce giant shock waves. The outlines of these waves have now been seen as radio-emitting structures.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.1133949</identifier><identifier>CODEN: SCIEAS</identifier><language>eng</language><publisher>Washington: American Association for the Advancement of Science</publisher><subject>Accretion ; Astronomy ; Cosmology ; Galaxies ; Galaxy clusters ; Mach number ; Magnetic fields ; Particle acceleration ; Particle energy ; Perspectives ; Radio telescopes ; Relativistic particles ; Shock waves ; Stars &amp; galaxies ; Thermal shock</subject><ispartof>Science (American Association for the Advancement of Science), 2006-11, Vol.314 (5800), p.772-773</ispartof><rights>Copyright 2006 American Association for the Advancement of Science</rights><rights>Copyright American Association for the Advancement of Science Nov 3, 2006</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c352t-d22213497611f82806f2b05e556a1c3aeefe9a9d7ad07694daab777757b24a183</citedby><cites>FETCH-LOGICAL-c352t-d22213497611f82806f2b05e556a1c3aeefe9a9d7ad07694daab777757b24a183</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/20031678$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/20031678$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>315,782,786,805,2888,2889,27933,27934,58026,58259</link.rule.ids></links><search><creatorcontrib>Enslin, Torsten A</creatorcontrib><title>Radio Traces of Cosmic Shock Waves</title><title>Science (American Association for the Advancement of Science)</title><description>Colliding and fusing galaxy clusters should produce giant shock waves. The outlines of these waves have now been seen as radio-emitting structures.</description><subject>Accretion</subject><subject>Astronomy</subject><subject>Cosmology</subject><subject>Galaxies</subject><subject>Galaxy clusters</subject><subject>Mach number</subject><subject>Magnetic fields</subject><subject>Particle acceleration</subject><subject>Particle energy</subject><subject>Perspectives</subject><subject>Radio telescopes</subject><subject>Relativistic particles</subject><subject>Shock waves</subject><subject>Stars &amp; galaxies</subject><subject>Thermal shock</subject><issn>0036-8075</issn><issn>1095-9203</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNqFkEtLAzEQgIMoWKtnT8LSg7e1mWTzOkrxBQVBKx7DbDaLW9umJlvBf2-kiwcvzmUY5pth5iPkHOgVAJPT5Dq_cT4XnJvKHJARUCNKwyg_JCNKuSw1VeKYnKS0pDT3DB-RyRM2XSgWEZ1PRWiLWUjrzhXPb8G9F6_46dMpOWpxlfzZkMfk5fZmMbsv5493D7Preem4YH3ZMMaAV0ZJgFYzTWXLaiq8EBLBcfS-9QZNo7ChSpqqQaxVDqFqViFoPiaX-73bGD52PvV23SXnVyvc-LBLlkvQlWDiXxAM15lTGZz8AZdhFzf5CZtPlUxJxjM03UMuhpSib-02dmuMXxao_TFrB7N2MJsnLvYTy9SH-Iuz7Bik0vwbK7Rziw</recordid><startdate>20061103</startdate><enddate>20061103</enddate><creator>Enslin, Torsten A</creator><general>American Association for the Advancement of Science</general><general>The American Association for the Advancement of Science</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7QF</scope><scope>7QG</scope><scope>7QL</scope><scope>7QP</scope><scope>7QQ</scope><scope>7QR</scope><scope>7SC</scope><scope>7SE</scope><scope>7SN</scope><scope>7SP</scope><scope>7SR</scope><scope>7SS</scope><scope>7T7</scope><scope>7TA</scope><scope>7TB</scope><scope>7TK</scope><scope>7TM</scope><scope>7U5</scope><scope>7U9</scope><scope>8BQ</scope><scope>8FD</scope><scope>C1K</scope><scope>F28</scope><scope>FR3</scope><scope>H8D</scope><scope>H8G</scope><scope>H94</scope><scope>JG9</scope><scope>JQ2</scope><scope>K9.</scope><scope>KR7</scope><scope>L7M</scope><scope>L~C</scope><scope>L~D</scope><scope>M7N</scope><scope>P64</scope><scope>RC3</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20061103</creationdate><title>Radio Traces of Cosmic Shock Waves</title><author>Enslin, Torsten A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c352t-d22213497611f82806f2b05e556a1c3aeefe9a9d7ad07694daab777757b24a183</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>Accretion</topic><topic>Astronomy</topic><topic>Cosmology</topic><topic>Galaxies</topic><topic>Galaxy clusters</topic><topic>Mach number</topic><topic>Magnetic fields</topic><topic>Particle acceleration</topic><topic>Particle energy</topic><topic>Perspectives</topic><topic>Radio telescopes</topic><topic>Relativistic particles</topic><topic>Shock waves</topic><topic>Stars &amp; galaxies</topic><topic>Thermal shock</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Enslin, Torsten A</creatorcontrib><collection>CrossRef</collection><collection>Aluminium Industry Abstracts</collection><collection>Animal Behavior Abstracts</collection><collection>Bacteriology Abstracts (Microbiology B)</collection><collection>Calcium &amp; Calcified Tissue Abstracts</collection><collection>Ceramic Abstracts</collection><collection>Chemoreception Abstracts</collection><collection>Computer and Information Systems Abstracts</collection><collection>Corrosion Abstracts</collection><collection>Ecology Abstracts</collection><collection>Electronics &amp; Communications Abstracts</collection><collection>Engineered Materials Abstracts</collection><collection>Entomology Abstracts (Full archive)</collection><collection>Industrial and Applied Microbiology Abstracts (Microbiology A)</collection><collection>Materials Business File</collection><collection>Mechanical &amp; Transportation Engineering Abstracts</collection><collection>Neurosciences Abstracts</collection><collection>Nucleic Acids Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Virology and AIDS Abstracts</collection><collection>METADEX</collection><collection>Technology Research Database</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ANTE: Abstracts in New Technology &amp; Engineering</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Copper Technical Reference Library</collection><collection>AIDS and Cancer Research Abstracts</collection><collection>Materials Research Database</collection><collection>ProQuest Computer Science Collection</collection><collection>ProQuest Health &amp; Medical Complete (Alumni)</collection><collection>Civil Engineering Abstracts</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Computer and Information Systems Abstracts – Academic</collection><collection>Computer and Information Systems Abstracts Professional</collection><collection>Algology Mycology and Protozoology Abstracts (Microbiology C)</collection><collection>Biotechnology and BioEngineering Abstracts</collection><collection>Genetics Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><jtitle>Science (American Association for the Advancement of Science)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Enslin, Torsten A</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Radio Traces of Cosmic Shock Waves</atitle><jtitle>Science (American Association for the Advancement of Science)</jtitle><date>2006-11-03</date><risdate>2006</risdate><volume>314</volume><issue>5800</issue><spage>772</spage><epage>773</epage><pages>772-773</pages><issn>0036-8075</issn><eissn>1095-9203</eissn><coden>SCIEAS</coden><abstract>Colliding and fusing galaxy clusters should produce giant shock waves. The outlines of these waves have now been seen as radio-emitting structures.</abstract><cop>Washington</cop><pub>American Association for the Advancement of Science</pub><doi>10.1126/science.1133949</doi><tpages>2</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0036-8075
ispartof Science (American Association for the Advancement of Science), 2006-11, Vol.314 (5800), p.772-773
issn 0036-8075
1095-9203
language eng
recordid cdi_proquest_miscellaneous_36184525
source American Association for the Advancement of Science; JSTOR
subjects Accretion
Astronomy
Cosmology
Galaxies
Galaxy clusters
Mach number
Magnetic fields
Particle acceleration
Particle energy
Perspectives
Radio telescopes
Relativistic particles
Shock waves
Stars & galaxies
Thermal shock
title Radio Traces of Cosmic Shock Waves
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-03T11%3A40%3A11IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-jstor_proqu&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Radio%20Traces%20of%20Cosmic%20Shock%20Waves&rft.jtitle=Science%20(American%20Association%20for%20the%20Advancement%20of%20Science)&rft.au=Enslin,%20Torsten%20A&rft.date=2006-11-03&rft.volume=314&rft.issue=5800&rft.spage=772&rft.epage=773&rft.pages=772-773&rft.issn=0036-8075&rft.eissn=1095-9203&rft.coden=SCIEAS&rft_id=info:doi/10.1126/science.1133949&rft_dat=%3Cjstor_proqu%3E20031678%3C/jstor_proqu%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=213627623&rft_id=info:pmid/&rft_jstor_id=20031678&rfr_iscdi=true