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A SEYFERT-2-LIKE SPECTRUM IN THE HIGH-MASS X-RAY BINARY MICROQUASAR V4641 SGR
We present an analysis of three archival Chandra observations of the black hole V4641 Sgr, performed during a decline into quiescence. The last two observations in the sequence can be modeled with a simple power law. The first spectrum, however, is remarkably similar to spectra observed in Seyfert-2...
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Published in: | Astrophysical journal. Letters 2014-05, Vol.786 (2), p.1-5 |
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description | We present an analysis of three archival Chandra observations of the black hole V4641 Sgr, performed during a decline into quiescence. The last two observations in the sequence can be modeled with a simple power law. The first spectrum, however, is remarkably similar to spectra observed in Seyfert-2 active galactic nuclei, which arise through a combination of obscuration and reflection from distant material. This spectrum of V4641 Sgr can be fit extremely well with a model including partial-covering absorption and distant reflection. This model recovers a [Gamma] [Asymptotically = to] 2.0 power-law incident spectrum, typical of black holes at low Eddington fractions. The implied geometry is plausible in a high-mass X-ray binary like V4641 Sgr, and may be as compelling as explanations invoking Doppler-split line pairs in a jet, and/or unusual Comptonization. We discuss potential implications and means of testing these models. |
doi_str_mv | 10.1088/2041-8205/786/2/L20 |
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We discuss potential implications and means of testing these models.</description><subject>ACCRETION DISKS</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Asymptotic properties</subject><subject>Binary stars</subject><subject>BLACK HOLES</subject><subject>Black holes (astronomy)</subject><subject>EMISSION SPECTRA</subject><subject>GALAXY NUCLEI</subject><subject>JETS</subject><subject>MASS</subject><subject>Microquasars</subject><subject>POTENTIALS</subject><subject>Power law</subject><subject>REFLECTION</subject><subject>SEYFERT GALAXIES</subject><subject>Spectra</subject><subject>X-RAY SPECTRA</subject><subject>X-ray stars</subject><issn>2041-8205</issn><issn>2041-8213</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><recordid>eNqNkc1Og0AURidGE2v1CdxM4sbNyPzAdFhiQwsRWgVq7GoyDEPEtKUydOHbS9PGtat7c7-TuzgfAPcEPxEshEOxS5Cg2HMmgjvUSSi-AKPzlbDLvx171-DG2i-MKeZEjEAawDxcz8KsQBQl8UsI89dwWmSrFMYLWEQhjOJ5hNIgz-EHyoI1fI4XQbaGaTzNlm-rIA8y-O5yl8B8nt2Cq1ptrLk7zzFYzcJiGqFkOY-nQYI0E6JHnhLK14QL7deecDUttauUKKkWrC6NVmziV8qfVILzSgmma04qw-mQl4qVFRuDh9Pf1vaNtLrpjf7U7W5ndC8pZdwTHA_U44nad-33wdhebhurzWajdqY9WEk4931CGeX_Qd3BGCZkQNkJ1V1rbWdque-arep-JMHy2IY8upZH13JoQ1I5tMF-Adm_dJ4</recordid><startdate>20140510</startdate><enddate>20140510</enddate><creator>Morningstar, Warren R</creator><creator>Miller, Jon M</creator><creator>Reynolds, M T</creator><creator>Maitra, Dipankar</creator><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/0000-0002-5153-0920</orcidid></search><sort><creationdate>20140510</creationdate><title>A SEYFERT-2-LIKE SPECTRUM IN THE HIGH-MASS X-RAY BINARY MICROQUASAR V4641 SGR</title><author>Morningstar, Warren R ; Miller, Jon M ; Reynolds, M T ; Maitra, Dipankar</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c388t-5a8a9c168c9f584c2bc4aa8b2c83fbeca379da97d866da83cf61de622c8ba3bd3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>ACCRETION DISKS</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>Asymptotic properties</topic><topic>Binary stars</topic><topic>BLACK HOLES</topic><topic>Black holes (astronomy)</topic><topic>EMISSION SPECTRA</topic><topic>GALAXY NUCLEI</topic><topic>JETS</topic><topic>MASS</topic><topic>Microquasars</topic><topic>POTENTIALS</topic><topic>Power law</topic><topic>REFLECTION</topic><topic>SEYFERT GALAXIES</topic><topic>Spectra</topic><topic>X-RAY SPECTRA</topic><topic>X-ray stars</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Morningstar, Warren R</creatorcontrib><creatorcontrib>Miller, Jon M</creatorcontrib><creatorcontrib>Reynolds, M T</creatorcontrib><creatorcontrib>Maitra, Dipankar</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>Astrophysical journal. Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Morningstar, Warren R</au><au>Miller, Jon M</au><au>Reynolds, M T</au><au>Maitra, Dipankar</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A SEYFERT-2-LIKE SPECTRUM IN THE HIGH-MASS X-RAY BINARY MICROQUASAR V4641 SGR</atitle><jtitle>Astrophysical journal. Letters</jtitle><date>2014-05-10</date><risdate>2014</risdate><volume>786</volume><issue>2</issue><spage>1</spage><epage>5</epage><pages>1-5</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>We present an analysis of three archival Chandra observations of the black hole V4641 Sgr, performed during a decline into quiescence. The last two observations in the sequence can be modeled with a simple power law. 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subjects | ACCRETION DISKS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Asymptotic properties Binary stars BLACK HOLES Black holes (astronomy) EMISSION SPECTRA GALAXY NUCLEI JETS MASS Microquasars POTENTIALS Power law REFLECTION SEYFERT GALAXIES Spectra X-RAY SPECTRA X-ray stars |
title | A SEYFERT-2-LIKE SPECTRUM IN THE HIGH-MASS X-RAY BINARY MICROQUASAR V4641 SGR |
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