Observations of variable and transient X-ray sources with the Ariel V sky survey experiment

Results obtained during the first six mos in orbit of ARIEL-5 with the Leicester Sky Survey are reviewed. Among 80 sources found by a scan of the Milky Way, 16 are new, and 11 UHURU sources in the scanned region are not detected. Some of these sources may be transient. The light curve of Cen X-3 in...

Full description

Saved in:
Bibliographic Details
Published in:Astrophysics and space science 1976-06, Vol.42 (1), p.143-159
Main Authors: Pounds, K. A., Cooke, B. A., Ricketts, M. J., Turner, M. J., Peacock, A., Eadie, G.
Format: Article
Language:English
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-c293t-af6c7e30ebf862fc925379acd734401d29824278b631dcfa48aa9be164bb3a863
cites cdi_FETCH-LOGICAL-c293t-af6c7e30ebf862fc925379acd734401d29824278b631dcfa48aa9be164bb3a863
container_end_page 159
container_issue 1
container_start_page 143
container_title Astrophysics and space science
container_volume 42
creator Pounds, K. A.
Cooke, B. A.
Ricketts, M. J.
Turner, M. J.
Peacock, A.
Eadie, G.
description Results obtained during the first six mos in orbit of ARIEL-5 with the Leicester Sky Survey are reviewed. Among 80 sources found by a scan of the Milky Way, 16 are new, and 11 UHURU sources in the scanned region are not detected. Some of these sources may be transient. The light curve of Cen X-3 in a binary cycle shows a dip between phases 0.5 and 0.75, and a secondary maximum at the center of the dip. The dip and the maximum become progressively weaker in the succeeding cycles. These features are interpreted in terms of the stellar wind accretion model. Cyg X-1 observation for 14 days gives a broad minimum around superior conjunction. Four bright transient sources of nova-like light curves have been observed. The light curves and the spectra are given for TrA X-1 (A1524-62) and Tau X-T (A0535 + 26).
doi_str_mv 10.1007/BF00645535
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_22510938</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>18462959</sourcerecordid><originalsourceid>FETCH-LOGICAL-c293t-af6c7e30ebf862fc925379acd734401d29824278b631dcfa48aa9be164bb3a863</originalsourceid><addsrcrecordid>eNqFkE9Lw0AUxBdRsFYvfoI9eRCi-y-b7LEWq0KhF5WCh_B285ZG06TuJq399kYqePQ0DPObB28IueTshjOW3d7NGNMqTWV6REY8zURilF4ekxFjTCVaseUpOYvxfbBGm2xE3hY2YthCV7VNpK2nWwgV2BopNCXtAjSxwqajyyTAnsa2Dw4j3VXdinYrpJNQYU1fafwYwj5scU_xa4OhWg-lc3LioY548atj8jK7f54-JvPFw9N0Mk-cMLJLwGuXoWRofa6Fd0akMjPgykwqxXgpTC6UyHKrJS-dB5UDGItcK2sl5FqOydXh7ia0nz3GrlhX0WFdQ4NtHwshUs6MzP8Fea60MKkZwOsD6EIbY0BfbIaXIOwLzoqfoYu_oeU3kgBwyA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>18462959</pqid></control><display><type>article</type><title>Observations of variable and transient X-ray sources with the Ariel V sky survey experiment</title><source>Springer LINK Archives</source><creator>Pounds, K. A. ; Cooke, B. A. ; Ricketts, M. J. ; Turner, M. J. ; Peacock, A. ; Eadie, G.</creator><creatorcontrib>Pounds, K. A. ; Cooke, B. A. ; Ricketts, M. J. ; Turner, M. J. ; Peacock, A. ; Eadie, G.</creatorcontrib><description>Results obtained during the first six mos in orbit of ARIEL-5 with the Leicester Sky Survey are reviewed. Among 80 sources found by a scan of the Milky Way, 16 are new, and 11 UHURU sources in the scanned region are not detected. Some of these sources may be transient. The light curve of Cen X-3 in a binary cycle shows a dip between phases 0.5 and 0.75, and a secondary maximum at the center of the dip. The dip and the maximum become progressively weaker in the succeeding cycles. These features are interpreted in terms of the stellar wind accretion model. Cyg X-1 observation for 14 days gives a broad minimum around superior conjunction. Four bright transient sources of nova-like light curves have been observed. The light curves and the spectra are given for TrA X-1 (A1524-62) and Tau X-T (A0535 + 26).</description><identifier>ISSN: 0004-640X</identifier><identifier>EISSN: 1572-946X</identifier><identifier>DOI: 10.1007/BF00645535</identifier><language>eng</language><ispartof>Astrophysics and space science, 1976-06, Vol.42 (1), p.143-159</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c293t-af6c7e30ebf862fc925379acd734401d29824278b631dcfa48aa9be164bb3a863</citedby><cites>FETCH-LOGICAL-c293t-af6c7e30ebf862fc925379acd734401d29824278b631dcfa48aa9be164bb3a863</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Pounds, K. A.</creatorcontrib><creatorcontrib>Cooke, B. A.</creatorcontrib><creatorcontrib>Ricketts, M. J.</creatorcontrib><creatorcontrib>Turner, M. J.</creatorcontrib><creatorcontrib>Peacock, A.</creatorcontrib><creatorcontrib>Eadie, G.</creatorcontrib><title>Observations of variable and transient X-ray sources with the Ariel V sky survey experiment</title><title>Astrophysics and space science</title><description>Results obtained during the first six mos in orbit of ARIEL-5 with the Leicester Sky Survey are reviewed. Among 80 sources found by a scan of the Milky Way, 16 are new, and 11 UHURU sources in the scanned region are not detected. Some of these sources may be transient. The light curve of Cen X-3 in a binary cycle shows a dip between phases 0.5 and 0.75, and a secondary maximum at the center of the dip. The dip and the maximum become progressively weaker in the succeeding cycles. These features are interpreted in terms of the stellar wind accretion model. Cyg X-1 observation for 14 days gives a broad minimum around superior conjunction. Four bright transient sources of nova-like light curves have been observed. The light curves and the spectra are given for TrA X-1 (A1524-62) and Tau X-T (A0535 + 26).</description><issn>0004-640X</issn><issn>1572-946X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1976</creationdate><recordtype>article</recordtype><recordid>eNqFkE9Lw0AUxBdRsFYvfoI9eRCi-y-b7LEWq0KhF5WCh_B285ZG06TuJq399kYqePQ0DPObB28IueTshjOW3d7NGNMqTWV6REY8zURilF4ekxFjTCVaseUpOYvxfbBGm2xE3hY2YthCV7VNpK2nWwgV2BopNCXtAjSxwqajyyTAnsa2Dw4j3VXdinYrpJNQYU1fafwYwj5scU_xa4OhWg-lc3LioY548atj8jK7f54-JvPFw9N0Mk-cMLJLwGuXoWRofa6Fd0akMjPgykwqxXgpTC6UyHKrJS-dB5UDGItcK2sl5FqOydXh7ia0nz3GrlhX0WFdQ4NtHwshUs6MzP8Fea60MKkZwOsD6EIbY0BfbIaXIOwLzoqfoYu_oeU3kgBwyA</recordid><startdate>197606</startdate><enddate>197606</enddate><creator>Pounds, K. A.</creator><creator>Cooke, B. A.</creator><creator>Ricketts, M. J.</creator><creator>Turner, M. J.</creator><creator>Peacock, A.</creator><creator>Eadie, G.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>197606</creationdate><title>Observations of variable and transient X-ray sources with the Ariel V sky survey experiment</title><author>Pounds, K. A. ; Cooke, B. A. ; Ricketts, M. J. ; Turner, M. J. ; Peacock, A. ; Eadie, G.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c293t-af6c7e30ebf862fc925379acd734401d29824278b631dcfa48aa9be164bb3a863</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1976</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pounds, K. A.</creatorcontrib><creatorcontrib>Cooke, B. A.</creatorcontrib><creatorcontrib>Ricketts, M. J.</creatorcontrib><creatorcontrib>Turner, M. J.</creatorcontrib><creatorcontrib>Peacock, A.</creatorcontrib><creatorcontrib>Eadie, G.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astrophysics and space science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Pounds, K. A.</au><au>Cooke, B. A.</au><au>Ricketts, M. J.</au><au>Turner, M. J.</au><au>Peacock, A.</au><au>Eadie, G.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Observations of variable and transient X-ray sources with the Ariel V sky survey experiment</atitle><jtitle>Astrophysics and space science</jtitle><date>1976-06</date><risdate>1976</risdate><volume>42</volume><issue>1</issue><spage>143</spage><epage>159</epage><pages>143-159</pages><issn>0004-640X</issn><eissn>1572-946X</eissn><abstract>Results obtained during the first six mos in orbit of ARIEL-5 with the Leicester Sky Survey are reviewed. Among 80 sources found by a scan of the Milky Way, 16 are new, and 11 UHURU sources in the scanned region are not detected. Some of these sources may be transient. The light curve of Cen X-3 in a binary cycle shows a dip between phases 0.5 and 0.75, and a secondary maximum at the center of the dip. The dip and the maximum become progressively weaker in the succeeding cycles. These features are interpreted in terms of the stellar wind accretion model. Cyg X-1 observation for 14 days gives a broad minimum around superior conjunction. Four bright transient sources of nova-like light curves have been observed. The light curves and the spectra are given for TrA X-1 (A1524-62) and Tau X-T (A0535 + 26).</abstract><doi>10.1007/BF00645535</doi><tpages>17</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0004-640X
ispartof Astrophysics and space science, 1976-06, Vol.42 (1), p.143-159
issn 0004-640X
1572-946X
language eng
recordid cdi_proquest_miscellaneous_22510938
source Springer LINK Archives
title Observations of variable and transient X-ray sources with the Ariel V sky survey experiment
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-04T19%3A25%3A56IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Observations%20of%20variable%20and%20transient%20X-ray%20sources%20with%20the%20Ariel%20V%20sky%20survey%20experiment&rft.jtitle=Astrophysics%20and%20space%20science&rft.au=Pounds,%20K.%20A.&rft.date=1976-06&rft.volume=42&rft.issue=1&rft.spage=143&rft.epage=159&rft.pages=143-159&rft.issn=0004-640X&rft.eissn=1572-946X&rft_id=info:doi/10.1007/BF00645535&rft_dat=%3Cproquest_cross%3E18462959%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c293t-af6c7e30ebf862fc925379acd734401d29824278b631dcfa48aa9be164bb3a863%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=18462959&rft_id=info:pmid/&rfr_iscdi=true