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Evidence of Radio Luminosity Evolution of Quasi-stellar Radio Sources
THE evolution of quasi-stellar radio sources has been studied by investigating the relationship between log N and log S , where N is the number of sources with flux density exceeding S (refs. 1–4), but this method does not distinguish between density evolution and luminosity evolution. A differentia...
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Published in: | Nature (London) 1970-01, Vol.225 (5230), p.358-359 |
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container_title | Nature (London) |
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creator | ARAKELIAN, M. A |
description | THE evolution of quasi-stellar radio sources has been studied by investigating the relationship between log
N
and log
S
, where
N
is the number of sources with flux density exceeding
S
(refs. 1–4), but this method does not distinguish between density evolution and luminosity evolution. A differential study of the optical and radio brightnesses of quasars may provide a method for determining the nature of their evolution. Density variation would be expressed both in the radio and optical wavelengths, while luminosity evolution may only be shown in the optical brightness. |
doi_str_mv | 10.1038/225358a0 |
format | article |
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N
and log
S
, where
N
is the number of sources with flux density exceeding
S
(refs. 1–4), but this method does not distinguish between density evolution and luminosity evolution. A differential study of the optical and radio brightnesses of quasars may provide a method for determining the nature of their evolution. Density variation would be expressed both in the radio and optical wavelengths, while luminosity evolution may only be shown in the optical brightness.</description><identifier>ISSN: 0028-0836</identifier><identifier>EISSN: 1476-4687</identifier><identifier>DOI: 10.1038/225358a0</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>Humanities and Social Sciences ; letter ; multidisciplinary ; Science</subject><ispartof>Nature (London), 1970-01, Vol.225 (5230), p.358-359</ispartof><rights>Springer Nature Limited 1970</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c311t-89036f382fd643906a3026e7a8030592f5c117db9b51fcff4e361aebae8958d83</citedby><cites>FETCH-LOGICAL-c311t-89036f382fd643906a3026e7a8030592f5c117db9b51fcff4e361aebae8958d83</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,2727,27924,27925</link.rule.ids></links><search><creatorcontrib>ARAKELIAN, M. A</creatorcontrib><title>Evidence of Radio Luminosity Evolution of Quasi-stellar Radio Sources</title><title>Nature (London)</title><addtitle>Nature</addtitle><description>THE evolution of quasi-stellar radio sources has been studied by investigating the relationship between log
N
and log
S
, where
N
is the number of sources with flux density exceeding
S
(refs. 1–4), but this method does not distinguish between density evolution and luminosity evolution. A differential study of the optical and radio brightnesses of quasars may provide a method for determining the nature of their evolution. Density variation would be expressed both in the radio and optical wavelengths, while luminosity evolution may only be shown in the optical brightness.</description><subject>Humanities and Social Sciences</subject><subject>letter</subject><subject>multidisciplinary</subject><subject>Science</subject><issn>0028-0836</issn><issn>1476-4687</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1970</creationdate><recordtype>article</recordtype><recordid>eNptz81KxDAUBeAgCtZR8AmkS11Ub5ImTZcydFQoiH_rkqaJZOgkkrQD8_Z26DgrV3dxPw7nIHSN4R4DFQ-EMMqEhBOU4LzgWc5FcYoSACIyEJSfo4sY1wDAcJEnqKq2ttNO6dSb9F121qf1uLHORzvs0mrr-3Gw3u2_b6OMNouD7nsZDvbDj0HpeInOjOyjvjrcBfpaVZ_L56x-fXpZPtaZohgPmSiBckMFMR3PaQlcUiBcF1IABVYSwxTGRdeWLcNGGZNryrHUrdSiZKITdIFu51wVfIxBm-Yn2I0MuwZDs5_f_M2f6N1M40Tctw7Neurqpnb_2ZvZOjmMQR9Dj-AXl6RjcQ</recordid><startdate>19700101</startdate><enddate>19700101</enddate><creator>ARAKELIAN, M. A</creator><general>Nature Publishing Group UK</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19700101</creationdate><title>Evidence of Radio Luminosity Evolution of Quasi-stellar Radio Sources</title><author>ARAKELIAN, M. A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c311t-89036f382fd643906a3026e7a8030592f5c117db9b51fcff4e361aebae8958d83</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1970</creationdate><topic>Humanities and Social Sciences</topic><topic>letter</topic><topic>multidisciplinary</topic><topic>Science</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>ARAKELIAN, M. A</creatorcontrib><collection>CrossRef</collection><jtitle>Nature (London)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>ARAKELIAN, M. A</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Evidence of Radio Luminosity Evolution of Quasi-stellar Radio Sources</atitle><jtitle>Nature (London)</jtitle><stitle>Nature</stitle><date>1970-01-01</date><risdate>1970</risdate><volume>225</volume><issue>5230</issue><spage>358</spage><epage>359</epage><pages>358-359</pages><issn>0028-0836</issn><eissn>1476-4687</eissn><abstract>THE evolution of quasi-stellar radio sources has been studied by investigating the relationship between log
N
and log
S
, where
N
is the number of sources with flux density exceeding
S
(refs. 1–4), but this method does not distinguish between density evolution and luminosity evolution. A differential study of the optical and radio brightnesses of quasars may provide a method for determining the nature of their evolution. Density variation would be expressed both in the radio and optical wavelengths, while luminosity evolution may only be shown in the optical brightness.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><doi>10.1038/225358a0</doi><tpages>2</tpages></addata></record> |
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language | eng |
recordid | cdi_crossref_primary_10_1038_225358a0 |
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subjects | Humanities and Social Sciences letter multidisciplinary Science |
title | Evidence of Radio Luminosity Evolution of Quasi-stellar Radio Sources |
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