Far-infrared-radio relation in cluster galaxies at intermediate redshift
The radio luminosities at 1.4 GHz is tightly correlated with the far-infrared luminosities for various galaxy types (e.g. [16, 6, 2]) over a wide range of redshift (see e.g. [5, 1, 15, 8, 7]). The relationship is widely believed to be driven by the internal star formation activity. Radio emission fr...
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| creator | Randriamampandry, Solohery M |
| description | The radio luminosities at 1.4 GHz is tightly correlated with the far-infrared
luminosities for various galaxy types (e.g. [16, 6, 2]) over a wide range of
redshift (see e.g. [5, 1, 15, 8, 7]). The relationship is widely believed to be
driven by the internal star formation activity. Radio emission from these
galaxies are predominantly produced from the synchrotron emission of cosmic-ray
electrons accelerated in supernova shocks. The infrared emission is due to
ultraviolet light from young massive stars that is absorbed and re-radiated by
dust [3]. A correlation is found also in local clusters but cluster galaxies
appears to have excess radio emission relative to the amount of far-infrared
emission [9, 13, 11]. In this work, we measure the far-infrared-radio
relationship in a massive cluster to test how this relationship changes at
intermediate z between the field and a high-density cluster environment. |
| doi_str_mv | 10.48550/arxiv.1604.00992 |
| format | Article |
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luminosities for various galaxy types (e.g. [16, 6, 2]) over a wide range of
redshift (see e.g. [5, 1, 15, 8, 7]). The relationship is widely believed to be
driven by the internal star formation activity. Radio emission from these
galaxies are predominantly produced from the synchrotron emission of cosmic-ray
electrons accelerated in supernova shocks. The infrared emission is due to
ultraviolet light from young massive stars that is absorbed and re-radiated by
dust [3]. A correlation is found also in local clusters but cluster galaxies
appears to have excess radio emission relative to the amount of far-infrared
emission [9, 13, 11]. In this work, we measure the far-infrared-radio
relationship in a massive cluster to test how this relationship changes at
intermediate z between the field and a high-density cluster environment.</description><identifier>DOI: 10.48550/arxiv.1604.00992</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies</subject><creationdate>2016-03</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/1604.00992$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.1604.00992$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Randriamampandry, Solohery M</creatorcontrib><title>Far-infrared-radio relation in cluster galaxies at intermediate redshift</title><description>The radio luminosities at 1.4 GHz is tightly correlated with the far-infrared
luminosities for various galaxy types (e.g. [16, 6, 2]) over a wide range of
redshift (see e.g. [5, 1, 15, 8, 7]). The relationship is widely believed to be
driven by the internal star formation activity. Radio emission from these
galaxies are predominantly produced from the synchrotron emission of cosmic-ray
electrons accelerated in supernova shocks. The infrared emission is due to
ultraviolet light from young massive stars that is absorbed and re-radiated by
dust [3]. A correlation is found also in local clusters but cluster galaxies
appears to have excess radio emission relative to the amount of far-infrared
emission [9, 13, 11]. In this work, we measure the far-infrared-radio
relationship in a massive cluster to test how this relationship changes at
intermediate z between the field and a high-density cluster environment.</description><subject>Physics - Astrophysics of Galaxies</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj81Kw0AURmfThVQfwJXzAhNnJvPTLKVYKxTcdB9uMnf0QprKzbS0b2-srj44fBw4QjwaXbmV9_oZ-ELnygTtKq2bxt6J7QZY0ZgZGJNiSHSUjAMUOo6SRtkPp6kgy08Y4EI4SSgznskBE0HB-ZymL8rlXiwyDBM-_O9S7Dev-_VW7T7e3tcvOwUhWmU1JOyd9yZa603oe-isbzDVKXYu1miC0S7oHMGnYALYVaedczl7G4yDeime_rS3lPab6QB8bX-T2ltS_QPJE0Z8</recordid><startdate>20160324</startdate><enddate>20160324</enddate><creator>Randriamampandry, Solohery M</creator><scope>GOX</scope></search><sort><creationdate>20160324</creationdate><title>Far-infrared-radio relation in cluster galaxies at intermediate redshift</title><author>Randriamampandry, Solohery M</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a672-20adec4551722516ccab259ed3d7b473e1610460f7a5d616a28b0444ff52614a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Physics - Astrophysics of Galaxies</topic><toplevel>online_resources</toplevel><creatorcontrib>Randriamampandry, Solohery M</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Randriamampandry, Solohery M</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Far-infrared-radio relation in cluster galaxies at intermediate redshift</atitle><date>2016-03-24</date><risdate>2016</risdate><abstract>The radio luminosities at 1.4 GHz is tightly correlated with the far-infrared
luminosities for various galaxy types (e.g. [16, 6, 2]) over a wide range of
redshift (see e.g. [5, 1, 15, 8, 7]). The relationship is widely believed to be
driven by the internal star formation activity. Radio emission from these
galaxies are predominantly produced from the synchrotron emission of cosmic-ray
electrons accelerated in supernova shocks. The infrared emission is due to
ultraviolet light from young massive stars that is absorbed and re-radiated by
dust [3]. A correlation is found also in local clusters but cluster galaxies
appears to have excess radio emission relative to the amount of far-infrared
emission [9, 13, 11]. In this work, we measure the far-infrared-radio
relationship in a massive cluster to test how this relationship changes at
intermediate z between the field and a high-density cluster environment.</abstract><doi>10.48550/arxiv.1604.00992</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Physics - Astrophysics of Galaxies |
| title | Far-infrared-radio relation in cluster galaxies at intermediate redshift |
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