Shot Noise in 3c 273
The underlying impulse sequence responsible for the optical variability displayed by 3C 273 is presented. The sequence is random and consistent with a shot-noise process in which the mean rate of events is 8 yr/sup -1/. The implication of the result for proposed physical models is briefly discussed....
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Veröffentlicht in: | Astrophys. J.; (United States) 1976-11, Vol.209, p.663 |
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container_title | Astrophys. J.; (United States) |
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creator | Fahlman, G. G. Ulrych, Tad J. |
description | The underlying impulse sequence responsible for the optical variability displayed by 3C 273 is presented. The sequence is random and consistent with a shot-noise process in which the mean rate of events is 8 yr/sup -1/. The implication of the result for proposed physical models is briefly discussed. (AIP) |
doi_str_mv | 10.1086/154765 |
format | Article |
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G. ; Ulrych, Tad J. ; Institute of Astronomy and Space Science, University of British Columbia</creatorcontrib><description>The underlying impulse sequence responsible for the optical variability displayed by 3C 273 is presented. The sequence is random and consistent with a shot-noise process in which the mean rate of events is 8 yr/sup -1/. The implication of the result for proposed physical models is briefly discussed. (AIP)</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1086/154765</identifier><language>eng</language><publisher>United States</publisher><subject>640103 - Astrophysics & Cosmology- Quasi-Stellar, Radio, & X-Ray Sources- (-1987) ; BACKGROUND RADIATION ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; COSMIC RADIATION ; COSMIC RADIO SOURCES ; IONIZING RADIATIONS ; MATHEMATICAL MODELS ; NEUTRON STARS ; NOISE ; PULSARS ; PULSATIONS ; QUASARS ; RADIATIONS ; STAR MODELS ; STARS ; STATISTICAL MODELS ; SUPERNOVA REMNANTS ; VARIATIONS</subject><ispartof>Astrophys. J.; (United States), 1976-11, Vol.209, p.663</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c180t-bacf13f63de293fce5d69e74896660b3e61e50a7634979a0162a09dbf361cc243</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,881,27901,27902</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/7137210$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Fahlman, G. G.</creatorcontrib><creatorcontrib>Ulrych, Tad J.</creatorcontrib><creatorcontrib>Institute of Astronomy and Space Science, University of British Columbia</creatorcontrib><title>Shot Noise in 3c 273</title><title>Astrophys. J.; (United States)</title><description>The underlying impulse sequence responsible for the optical variability displayed by 3C 273 is presented. The sequence is random and consistent with a shot-noise process in which the mean rate of events is 8 yr/sup -1/. The implication of the result for proposed physical models is briefly discussed. (AIP)</description><subject>640103 - Astrophysics & Cosmology- Quasi-Stellar, Radio, & X-Ray Sources- (-1987)</subject><subject>BACKGROUND RADIATION</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>COSMIC RADIATION</subject><subject>COSMIC RADIO SOURCES</subject><subject>IONIZING RADIATIONS</subject><subject>MATHEMATICAL MODELS</subject><subject>NEUTRON STARS</subject><subject>NOISE</subject><subject>PULSARS</subject><subject>PULSATIONS</subject><subject>QUASARS</subject><subject>RADIATIONS</subject><subject>STAR MODELS</subject><subject>STARS</subject><subject>STATISTICAL MODELS</subject><subject>SUPERNOVA REMNANTS</subject><subject>VARIATIONS</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1976</creationdate><recordtype>article</recordtype><recordid>eNotj8FKxDAURYMoWEdd-QHFhbvoe3nJS7OUwVFh0IUK7kKaJkxFW2m68e91qKvLhcOBI8Q5wjVCwzdotGVzICo01EhNxh6KCgC0ZLLvx-KklI_9Vc5V4uJlN87109iXVPdDTbFWlk7FUQ6fJZ3970q8be5e1w9y-3z_uL7dyogNzLINMSNlpi4pRzkm07FLVjeOmaGlxJgMBMuknXUBkFUA17WZGGNUmlbicvGOZe59if2c4i6Ow5Di7C2SVQh_0NUCxWksZUrZf0_9V5h-PILfB_slmH4B_itDMA</recordid><startdate>19761101</startdate><enddate>19761101</enddate><creator>Fahlman, G. G.</creator><creator>Ulrych, Tad J.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>19761101</creationdate><title>Shot Noise in 3c 273</title><author>Fahlman, G. G. ; Ulrych, Tad J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c180t-bacf13f63de293fce5d69e74896660b3e61e50a7634979a0162a09dbf361cc243</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1976</creationdate><topic>640103 - Astrophysics & Cosmology- Quasi-Stellar, Radio, & X-Ray Sources- (-1987)</topic><topic>BACKGROUND RADIATION</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>COSMIC RADIATION</topic><topic>COSMIC RADIO SOURCES</topic><topic>IONIZING RADIATIONS</topic><topic>MATHEMATICAL MODELS</topic><topic>NEUTRON STARS</topic><topic>NOISE</topic><topic>PULSARS</topic><topic>PULSATIONS</topic><topic>QUASARS</topic><topic>RADIATIONS</topic><topic>STAR MODELS</topic><topic>STARS</topic><topic>STATISTICAL MODELS</topic><topic>SUPERNOVA REMNANTS</topic><topic>VARIATIONS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Fahlman, G. G.</creatorcontrib><creatorcontrib>Ulrych, Tad J.</creatorcontrib><creatorcontrib>Institute of Astronomy and Space Science, University of British Columbia</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Astrophys. J.; (United States)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Fahlman, G. G.</au><au>Ulrych, Tad J.</au><aucorp>Institute of Astronomy and Space Science, University of British Columbia</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Shot Noise in 3c 273</atitle><jtitle>Astrophys. J.; (United States)</jtitle><date>1976-11-01</date><risdate>1976</risdate><volume>209</volume><spage>663</spage><pages>663-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>The underlying impulse sequence responsible for the optical variability displayed by 3C 273 is presented. The sequence is random and consistent with a shot-noise process in which the mean rate of events is 8 yr/sup -1/. The implication of the result for proposed physical models is briefly discussed. (AIP)</abstract><cop>United States</cop><doi>10.1086/154765</doi></addata></record> |
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subjects | 640103 - Astrophysics & Cosmology- Quasi-Stellar, Radio, & X-Ray Sources- (-1987) BACKGROUND RADIATION CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMIC RADIATION COSMIC RADIO SOURCES IONIZING RADIATIONS MATHEMATICAL MODELS NEUTRON STARS NOISE PULSARS PULSATIONS QUASARS RADIATIONS STAR MODELS STARS STATISTICAL MODELS SUPERNOVA REMNANTS VARIATIONS |
title | Shot Noise in 3c 273 |
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