Loading…

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...

Full description

Saved in:
Bibliographic Details
Published in:Nature (London) 1970-01, Vol.225 (5230), p.358-359
Main Author: ARAKELIAN, M. A
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c311t-89036f382fd643906a3026e7a8030592f5c117db9b51fcff4e361aebae8958d83
cites cdi_FETCH-LOGICAL-c311t-89036f382fd643906a3026e7a8030592f5c117db9b51fcff4e361aebae8958d83
container_end_page 359
container_issue 5230
container_start_page 358
container_title Nature (London)
container_volume 225
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
fullrecord <record><control><sourceid>nature_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1038_225358a0</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>225358a0</sourcerecordid><originalsourceid>FETCH-LOGICAL-c311t-89036f382fd643906a3026e7a8030592f5c117db9b51fcff4e361aebae8958d83</originalsourceid><addsrcrecordid>eNptz81KxDAUBeAgCtZR8AmkS11Ub5ImTZcydFQoiH_rkqaJZOgkkrQD8_Z26DgrV3dxPw7nIHSN4R4DFQ-EMMqEhBOU4LzgWc5FcYoSACIyEJSfo4sY1wDAcJEnqKq2ttNO6dSb9F121qf1uLHORzvs0mrr-3Gw3u2_b6OMNouD7nsZDvbDj0HpeInOjOyjvjrcBfpaVZ_L56x-fXpZPtaZohgPmSiBckMFMR3PaQlcUiBcF1IABVYSwxTGRdeWLcNGGZNryrHUrdSiZKITdIFu51wVfIxBm-Yn2I0MuwZDs5_f_M2f6N1M40Tctw7Neurqpnb_2ZvZOjmMQR9Dj-AXl6RjcQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Evidence of Radio Luminosity Evolution of Quasi-stellar Radio Sources</title><source>Nature</source><creator>ARAKELIAN, M. A</creator><creatorcontrib>ARAKELIAN, M. A</creatorcontrib><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><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>
fulltext fulltext
identifier ISSN: 0028-0836
ispartof Nature (London), 1970-01, Vol.225 (5230), p.358-359
issn 0028-0836
1476-4687
language eng
recordid cdi_crossref_primary_10_1038_225358a0
source Nature
subjects Humanities and Social Sciences
letter
multidisciplinary
Science
title Evidence of Radio Luminosity Evolution of Quasi-stellar Radio Sources
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-02T17%3A38%3A02IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-nature_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Evidence%20of%20Radio%20Luminosity%20Evolution%20of%20Quasi-stellar%20Radio%20Sources&rft.jtitle=Nature%20(London)&rft.au=ARAKELIAN,%20M.%20A&rft.date=1970-01-01&rft.volume=225&rft.issue=5230&rft.spage=358&rft.epage=359&rft.pages=358-359&rft.issn=0028-0836&rft.eissn=1476-4687&rft_id=info:doi/10.1038/225358a0&rft_dat=%3Cnature_cross%3E225358a0%3C/nature_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c311t-89036f382fd643906a3026e7a8030592f5c117db9b51fcff4e361aebae8958d83%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true