LONG-TERM MONITORING OF THE BLACK HOLE CANDIDATE SWIFT J1753.5-0127 WITH INTEGRAL/SPI
ABSTRACT The black hole candidate (BHC) Swift J1753.5-0127 went into outburst in 2005 June. Rather than fade into quiescence as most BHC transients do, it has remained in a low hard spectral state for most of the ∼9 years after its outburst. Its persistent emission during the hard state is reminisce...
Gespeichert in:
| Veröffentlicht in: | The Astrophysical journal 2015-07, Vol.807 (1), p.1-7 |
|---|---|
| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext bestellen |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 7 |
|---|---|
| container_issue | 1 |
| container_start_page | 1 |
| container_title | The Astrophysical journal |
| container_volume | 807 |
| creator | Rodi, J. Jourdain, E. Roques, J. P. |
| description | ABSTRACT The black hole candidate (BHC) Swift J1753.5-0127 went into outburst in 2005 June. Rather than fade into quiescence as most BHC transients do, it has remained in a low hard spectral state for most of the ∼9 years after its outburst. Its persistent emission during the hard state is reminiscent of the black hole Cyg X-1 and the BHCs 1E 1740.7-2942 and GRS 1758-258. Thus far, hard X-ray/soft gamma-ray results have mainly focused on the 2005 flare, with a few additional observations during 2007. Here, we present results from INTEGRAL/SPI observations from 2005-2010 spanning the 22-650 keV energy range. Spectral analysis shows a weak high-energy excess ( ) above a cutoff power-law model that is well fit by a power law, suggesting an additional spectral component. Observations of Cyg X-1, 1E 1740.7-2942, and GRS 1758-258 have shown similar spectra requiring an additional high-energy component. The SPI results are compared to previously reported results for Swift J1753.5-0127 as well as observations of other sources. |
| doi_str_mv | 10.1088/0004-637X/807/1/106 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_proquest_miscellaneous_1765948303</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1765948303</sourcerecordid><originalsourceid>FETCH-LOGICAL-c413t-141e7ddf6d80464952f930a92db76ce1d233a19ad3fd930b40f052566661120b3</originalsourceid><addsrcrecordid>eNqN0U1LwzAYB_AgCs6XT-AlIIKX2jxJ-pJjnd1Wra1sHXoLXZtix1xr0x389qZM9CLicwlJfnkC_wehCyA3QHzfJoRwy2Xei-0TzwYbiHuARuAw3-LM8Q7R6FscoxOt18OWCjFCyzhNplYWzh_xY5pEWTqPkilOJzibhfg2DsYPeJbGIR4HyV10F2QhXjxHkwzfg-ewG8ciQD38HGUzHCVZOJ0Hsb14is7QUZVvtDr_Wk_RchJm45kVp9NoHMRWwYH1FnBQXllWbukT7nLh0Eowkgtarjy3UFBSxnIQecmq0lysOKmIQx3XFAAlK3aKLvd9G93XUhd1r4rXotluVdFLSn2fCk6Mut6rtmved0r38q3Whdps8q1qdlqCJxg1xdx_UNcR3GeEGcr2tOgarTtVybar3_LuQwKRw1TkELIcMpdmKhLM4fDB1f5V3bRy3ey6rclH5u36x8i2rIyzf3F_df4EW-qPSA</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1765948303</pqid></control><display><type>article</type><title>LONG-TERM MONITORING OF THE BLACK HOLE CANDIDATE SWIFT J1753.5-0127 WITH INTEGRAL/SPI</title><source>Institute of Physics Open Access Journal Titles</source><creator>Rodi, J. ; Jourdain, E. ; Roques, J. P.</creator><creatorcontrib>Rodi, J. ; Jourdain, E. ; Roques, J. P.</creatorcontrib><description>ABSTRACT The black hole candidate (BHC) Swift J1753.5-0127 went into outburst in 2005 June. Rather than fade into quiescence as most BHC transients do, it has remained in a low hard spectral state for most of the ∼9 years after its outburst. Its persistent emission during the hard state is reminiscent of the black hole Cyg X-1 and the BHCs 1E 1740.7-2942 and GRS 1758-258. Thus far, hard X-ray/soft gamma-ray results have mainly focused on the 2005 flare, with a few additional observations during 2007. Here, we present results from INTEGRAL/SPI observations from 2005-2010 spanning the 22-650 keV energy range. Spectral analysis shows a weak high-energy excess ( ) above a cutoff power-law model that is well fit by a power law, suggesting an additional spectral component. Observations of Cyg X-1, 1E 1740.7-2942, and GRS 1758-258 have shown similar spectra requiring an additional high-energy component. The SPI results are compared to previously reported results for Swift J1753.5-0127 as well as observations of other sources.</description><identifier>ISSN: 0004-637X</identifier><identifier>ISSN: 1538-4357</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/807/1/106</identifier><language>eng</language><publisher>United Kingdom: The American Astronomical Society</publisher><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; black hole physics ; BLACK HOLES ; Black holes (astronomy) ; COMPARATIVE EVALUATIONS ; EMISSION ; Flares ; GAMMA RADIATION ; HARD X RADIATION ; Integrals ; Monitoring ; Outbursts ; SPECTRA ; X-rays ; X-rays: binaries ; X-rays: individual (Swift J1753.5-0127)</subject><ispartof>The Astrophysical journal, 2015-07, Vol.807 (1), p.1-7</ispartof><rights>2015. The American Astronomical Society. All rights reserved.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c413t-141e7ddf6d80464952f930a92db76ce1d233a19ad3fd930b40f052566661120b3</citedby><cites>FETCH-LOGICAL-c413t-141e7ddf6d80464952f930a92db76ce1d233a19ad3fd930b40f052566661120b3</cites><orcidid>0000-0003-2126-5908</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/0004-637X/807/1/106/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>230,314,776,780,881,27901,27902,38867,53842</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.1088/0004-637X/807/1/106$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttps://www.osti.gov/biblio/22882940$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Rodi, J.</creatorcontrib><creatorcontrib>Jourdain, E.</creatorcontrib><creatorcontrib>Roques, J. P.</creatorcontrib><title>LONG-TERM MONITORING OF THE BLACK HOLE CANDIDATE SWIFT J1753.5-0127 WITH INTEGRAL/SPI</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>ABSTRACT The black hole candidate (BHC) Swift J1753.5-0127 went into outburst in 2005 June. Rather than fade into quiescence as most BHC transients do, it has remained in a low hard spectral state for most of the ∼9 years after its outburst. Its persistent emission during the hard state is reminiscent of the black hole Cyg X-1 and the BHCs 1E 1740.7-2942 and GRS 1758-258. Thus far, hard X-ray/soft gamma-ray results have mainly focused on the 2005 flare, with a few additional observations during 2007. Here, we present results from INTEGRAL/SPI observations from 2005-2010 spanning the 22-650 keV energy range. Spectral analysis shows a weak high-energy excess ( ) above a cutoff power-law model that is well fit by a power law, suggesting an additional spectral component. Observations of Cyg X-1, 1E 1740.7-2942, and GRS 1758-258 have shown similar spectra requiring an additional high-energy component. The SPI results are compared to previously reported results for Swift J1753.5-0127 as well as observations of other sources.</description><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>black hole physics</subject><subject>BLACK HOLES</subject><subject>Black holes (astronomy)</subject><subject>COMPARATIVE EVALUATIONS</subject><subject>EMISSION</subject><subject>Flares</subject><subject>GAMMA RADIATION</subject><subject>HARD X RADIATION</subject><subject>Integrals</subject><subject>Monitoring</subject><subject>Outbursts</subject><subject>SPECTRA</subject><subject>X-rays</subject><subject>X-rays: binaries</subject><subject>X-rays: individual (Swift J1753.5-0127)</subject><issn>0004-637X</issn><issn>1538-4357</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqN0U1LwzAYB_AgCs6XT-AlIIKX2jxJ-pJjnd1Wra1sHXoLXZtix1xr0x389qZM9CLicwlJfnkC_wehCyA3QHzfJoRwy2Xei-0TzwYbiHuARuAw3-LM8Q7R6FscoxOt18OWCjFCyzhNplYWzh_xY5pEWTqPkilOJzibhfg2DsYPeJbGIR4HyV10F2QhXjxHkwzfg-ewG8ciQD38HGUzHCVZOJ0Hsb14is7QUZVvtDr_Wk_RchJm45kVp9NoHMRWwYH1FnBQXllWbukT7nLh0Eowkgtarjy3UFBSxnIQecmq0lysOKmIQx3XFAAlK3aKLvd9G93XUhd1r4rXotluVdFLSn2fCk6Mut6rtmved0r38q3Whdps8q1qdlqCJxg1xdx_UNcR3GeEGcr2tOgarTtVybar3_LuQwKRw1TkELIcMpdmKhLM4fDB1f5V3bRy3ey6rclH5u36x8i2rIyzf3F_df4EW-qPSA</recordid><startdate>20150701</startdate><enddate>20150701</enddate><creator>Rodi, J.</creator><creator>Jourdain, E.</creator><creator>Roques, J. P.</creator><general>The American Astronomical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0003-2126-5908</orcidid></search><sort><creationdate>20150701</creationdate><title>LONG-TERM MONITORING OF THE BLACK HOLE CANDIDATE SWIFT J1753.5-0127 WITH INTEGRAL/SPI</title><author>Rodi, J. ; Jourdain, E. ; Roques, J. P.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c413t-141e7ddf6d80464952f930a92db76ce1d233a19ad3fd930b40f052566661120b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>black hole physics</topic><topic>BLACK HOLES</topic><topic>Black holes (astronomy)</topic><topic>COMPARATIVE EVALUATIONS</topic><topic>EMISSION</topic><topic>Flares</topic><topic>GAMMA RADIATION</topic><topic>HARD X RADIATION</topic><topic>Integrals</topic><topic>Monitoring</topic><topic>Outbursts</topic><topic>SPECTRA</topic><topic>X-rays</topic><topic>X-rays: binaries</topic><topic>X-rays: individual (Swift J1753.5-0127)</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Rodi, J.</creatorcontrib><creatorcontrib>Jourdain, E.</creatorcontrib><creatorcontrib>Roques, J. P.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Rodi, J.</au><au>Jourdain, E.</au><au>Roques, J. P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>LONG-TERM MONITORING OF THE BLACK HOLE CANDIDATE SWIFT J1753.5-0127 WITH INTEGRAL/SPI</atitle><jtitle>The Astrophysical journal</jtitle><stitle>APJ</stitle><addtitle>Astrophys. J</addtitle><date>2015-07-01</date><risdate>2015</risdate><volume>807</volume><issue>1</issue><spage>1</spage><epage>7</epage><pages>1-7</pages><issn>0004-637X</issn><issn>1538-4357</issn><eissn>1538-4357</eissn><abstract>ABSTRACT The black hole candidate (BHC) Swift J1753.5-0127 went into outburst in 2005 June. Rather than fade into quiescence as most BHC transients do, it has remained in a low hard spectral state for most of the ∼9 years after its outburst. Its persistent emission during the hard state is reminiscent of the black hole Cyg X-1 and the BHCs 1E 1740.7-2942 and GRS 1758-258. Thus far, hard X-ray/soft gamma-ray results have mainly focused on the 2005 flare, with a few additional observations during 2007. Here, we present results from INTEGRAL/SPI observations from 2005-2010 spanning the 22-650 keV energy range. Spectral analysis shows a weak high-energy excess ( ) above a cutoff power-law model that is well fit by a power law, suggesting an additional spectral component. Observations of Cyg X-1, 1E 1740.7-2942, and GRS 1758-258 have shown similar spectra requiring an additional high-energy component. The SPI results are compared to previously reported results for Swift J1753.5-0127 as well as observations of other sources.</abstract><cop>United Kingdom</cop><pub>The American Astronomical Society</pub><doi>10.1088/0004-637X/807/1/106</doi><tpages>7</tpages><orcidid>https://orcid.org/0000-0003-2126-5908</orcidid></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | ISSN: 0004-637X |
| ispartof | The Astrophysical journal, 2015-07, Vol.807 (1), p.1-7 |
| issn | 0004-637X 1538-4357 1538-4357 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_1765948303 |
| source | Institute of Physics Open Access Journal Titles |
| subjects | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY black hole physics BLACK HOLES Black holes (astronomy) COMPARATIVE EVALUATIONS EMISSION Flares GAMMA RADIATION HARD X RADIATION Integrals Monitoring Outbursts SPECTRA X-rays X-rays: binaries X-rays: individual (Swift J1753.5-0127) |
| title | LONG-TERM MONITORING OF THE BLACK HOLE CANDIDATE SWIFT J1753.5-0127 WITH INTEGRAL/SPI |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-31T20%3A53%3A48IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=LONG-TERM%20MONITORING%20OF%20THE%20BLACK%20HOLE%20CANDIDATE%20SWIFT%20J1753.5-0127%20WITH%20INTEGRAL/SPI&rft.jtitle=The%20Astrophysical%20journal&rft.au=Rodi,%20J.&rft.date=2015-07-01&rft.volume=807&rft.issue=1&rft.spage=1&rft.epage=7&rft.pages=1-7&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.1088/0004-637X/807/1/106&rft_dat=%3Cproquest_O3W%3E1765948303%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1765948303&rft_id=info:pmid/&rfr_iscdi=true |