Long time-scale variability in GRS 1915+105
ABSTRACT We present very high resolution hydrodynamical simulations of accretion discs in black hole X‐ray binaries accreting near the Eddington limit. The results show that mass loss, irradiation and tidal interactions all have a profound effect on the observed behaviour of long‐period X‐ray transi...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2004-10, Vol.353 (4), p.1048-1054 |
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| container_issue | 4 |
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| container_title | Monthly notices of the Royal Astronomical Society |
| container_volume | 353 |
| creator | Truss, M. R. Wynn, G. A. |
| description | ABSTRACT
We present very high resolution hydrodynamical simulations of accretion discs in black hole X‐ray binaries accreting near the Eddington limit. The results show that mass loss, irradiation and tidal interactions all have a profound effect on the observed behaviour of long‐period X‐ray transients. In particular, the interplay of all of these effects in the outer regions of the accretion disc is able to drive long time‐scale (weeks to years) variability is these objects, and is a possible origin for some of the extreme variability of GRS 1915+105. |
| doi_str_mv | 10.1111/j.1365-2966.2004.08153.x |
| format | Article |
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We present very high resolution hydrodynamical simulations of accretion discs in black hole X‐ray binaries accreting near the Eddington limit. The results show that mass loss, irradiation and tidal interactions all have a profound effect on the observed behaviour of long‐period X‐ray transients. In particular, the interplay of all of these effects in the outer regions of the accretion disc is able to drive long time‐scale (weeks to years) variability is these objects, and is a possible origin for some of the extreme variability of GRS 1915+105.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1111/j.1365-2966.2004.08153.x</identifier><identifier>CODEN: MNRAA4</identifier><language>eng</language><publisher>23 Ainslie Place , Edinburgh EH3 6AJ , UK . Telephone 226 7232 Fax 226 3803: Blackwell Science Ltd</publisher><subject>accretion ; accretion discs ; accretion, accretion discs ; binaries: close ; stars: individual: GRS 1915+105</subject><ispartof>Monthly notices of the Royal Astronomical Society, 2004-10, Vol.353 (4), p.1048-1054</ispartof><rights>2004 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c4603-6d236239cf8c39dff418a20fe7095f7a8dce50c16eda022f3bf623a8346a79913</citedby><cites>FETCH-LOGICAL-c4603-6d236239cf8c39dff418a20fe7095f7a8dce50c16eda022f3bf623a8346a79913</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1111%2Fj.1365-2966.2004.08153.x$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1111%2Fj.1365-2966.2004.08153.x$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>315,781,785,1418,27929,27930,45579,45580</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=16195513$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Truss, M. R.</creatorcontrib><creatorcontrib>Wynn, G. A.</creatorcontrib><title>Long time-scale variability in GRS 1915+105</title><title>Monthly notices of the Royal Astronomical Society</title><description>ABSTRACT
We present very high resolution hydrodynamical simulations of accretion discs in black hole X‐ray binaries accreting near the Eddington limit. The results show that mass loss, irradiation and tidal interactions all have a profound effect on the observed behaviour of long‐period X‐ray transients. In particular, the interplay of all of these effects in the outer regions of the accretion disc is able to drive long time‐scale (weeks to years) variability is these objects, and is a possible origin for some of the extreme variability of GRS 1915+105.</description><subject>accretion</subject><subject>accretion discs</subject><subject>accretion, accretion discs</subject><subject>binaries: close</subject><subject>stars: individual: GRS 1915+105</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</creationdate><recordtype>article</recordtype><recordid>eNqNkE9PwyAcQInRxDn9Dr3oZWnlT6Fw8GAWncY5k6nzSBgFw-zaCZ1u397WLvMqF0h470d4AEQIJqhZl4sEEUZjLBhLMIRpAjmiJNkcgN7-4hD0ICQ05hlCx-AkhAVsSIJZDwzGVfke1W5p4qBVYaIv5Z2au8LV28iV0Wj6HCGB6ABBegqOrCqCOdvtffB6e_MyvIvHT6P74fU41imDJGY5JgwToS3XROTWpogrDK3JoKA2UzzXhkKNmMkVxNiSuW1wxUnKVCYEIn1w0c1d-epzbUItly5oUxSqNNU6SMwxzCjjDcg7UPsqBG-sXHm3VH4rEZRtHbmQbQTZRpBtHflbR24a9Xz3hmr_bb0qtQt_PkOCUkQa7qrjvl1htv-eLx8n0_bU-HHnu1Cbzd5X_kOyjGRUvk1GkuKHmUjJVM7ID7Rbg2U</recordid><startdate>200410</startdate><enddate>200410</enddate><creator>Truss, M. R.</creator><creator>Wynn, G. A.</creator><general>Blackwell Science Ltd</general><general>Blackwell Science</general><scope>BSCLL</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>200410</creationdate><title>Long time-scale variability in GRS 1915+105</title><author>Truss, M. R. ; Wynn, G. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4603-6d236239cf8c39dff418a20fe7095f7a8dce50c16eda022f3bf623a8346a79913</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2004</creationdate><topic>accretion</topic><topic>accretion discs</topic><topic>accretion, accretion discs</topic><topic>binaries: close</topic><topic>stars: individual: GRS 1915+105</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Truss, M. R.</creatorcontrib><creatorcontrib>Wynn, G. A.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Truss, M. R.</au><au>Wynn, G. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Long time-scale variability in GRS 1915+105</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>2004-10</date><risdate>2004</risdate><volume>353</volume><issue>4</issue><spage>1048</spage><epage>1054</epage><pages>1048-1054</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><coden>MNRAA4</coden><abstract>ABSTRACT
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| ispartof | Monthly notices of the Royal Astronomical Society, 2004-10, Vol.353 (4), p.1048-1054 |
| issn | 0035-8711 1365-2966 |
| language | eng |
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| source | Wiley Online Library - AutoHoldings Journals; Access via Oxford University Press (Open Access Collection) |
| subjects | accretion accretion discs accretion, accretion discs binaries: close stars: individual: GRS 1915+105 |
| title | Long time-scale variability in GRS 1915+105 |
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