On the fate of gas accreting at a low rate on to a black hole
Identifieur interne : 000555 ( Main/Exploration ); précédent : 000554; suivant : 000556On the fate of gas accreting at a low rate on to a black hole
Auteurs : Roger D. Blandford [États-Unis] ; Mitchell C. Begelman [États-Unis]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 1999-02-11.
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Abstract
Gas supplied conservatively to a black hole at rates well below the Eddington rate may not be able to radiate effectively and the net energy flux, including the energy transported by the viscous torque, is likely to be close to zero at all radii. This has the consequence that the gas accretes with positive energy so that it may escape. Accordingly, we propose that only a small fraction of the gas supplied actually falls on to the black hole, and that the binding energy it releases is transported radially outward by the torque so as to drive away the remainder in the form of a wind. This is a generalization of and an alternative to an ‘ADAF’ solution. Some observational implications and possible ways to distinguish these two types of flow are briefly discussed.
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DOI: 10.1046/j.1365-8711.1999.02358.x
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Soc.</title><idno type="ISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><imprint><publisher>Blackwell Science Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="1999-02-11">1999-02-11</date><biblScope unit="volume">303</biblScope><biblScope unit="issue">1</biblScope><biblScope unit="page" from="L1">L1</biblScope><biblScope unit="page" to="L5">L5</biblScope></imprint><idno type="ISSN">0035-8711</idno></series><idno type="istex">7409F6B778C2D070CDF454F1AE5757E0AD57DBEF</idno><idno type="DOI">10.1046/j.1365-8711.1999.02358.x</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>accretion, accretion discs</term><term>black hole physics</term><term>hydrodynamics</term></keywords></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract">Gas supplied conservatively to a black hole at rates well below the Eddington rate may not be able to radiate effectively and the net energy flux, including the energy transported by the viscous torque, is likely to be close to zero at all radii. This has the consequence that the gas accretes with positive energy so that it may escape. Accordingly, we propose that only a small fraction of the gas supplied actually falls on to the black hole, and that the binding energy it releases is transported radially outward by the torque so as to drive away the remainder in the form of a wind. This is a generalization of and an alternative to an ‘ADAF’ solution. Some observational implications and possible ways to distinguish these two types of flow are briefly discussed.</div></front></TEI><affiliations><list><country><li>États-Unis</li></country></list><tree><country name="États-Unis"><noRegion><name sortKey="Blandford, Roger D" sort="Blandford, Roger D" uniqKey="Blandford R" first="Roger D." last="Blandford">Roger D. Blandford</name></noRegion><name sortKey="Begelman, Mitchell C" sort="Begelman, Mitchell C" uniqKey="Begelman M" first="Mitchell C." last="Begelman">Mitchell C. Begelman</name><name sortKey="Begelman, Mitchell C" sort="Begelman, Mitchell C" uniqKey="Begelman M" first="Mitchell C." last="Begelman">Mitchell C. Begelman</name><name sortKey="Begelman, Mitchell C" sort="Begelman, Mitchell C" uniqKey="Begelman M" first="Mitchell C." last="Begelman">Mitchell C. Begelman</name><name sortKey="Blandford, Roger D" sort="Blandford, Roger D" uniqKey="Blandford R" first="Roger D." last="Blandford">Roger D. Blandford</name></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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