Eddington capture sphere around luminous stars
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F12%3A%230004527" target="_blank" >RIV/47813059:19240/12:#0004527 - isvavai.cz</a>
Result on the web
<a href="http://www.aanda.org/index.php?option=com_article&access=doi&doi=10.1051/0004-6361/201220187&Itemid=129" target="_blank" >http://www.aanda.org/index.php?option=com_article&access=doi&doi=10.1051/0004-6361/201220187&Itemid=129</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201220187" target="_blank" >10.1051/0004-6361/201220187</a>
Alternative languages
Result language
angličtina
Original language name
Eddington capture sphere around luminous stars
Original language description
Test particles infalling from infinity onto a compact spherical star with a mildly super-Eddington luminosity at its surface are typically trapped on the "Eddington capture sphere" and do not reach the surface of the star. The presence of a sphere on which radiation pressure balances gravity for static particles was first discovered some twenty five years ago. Subsequently, it was shown to be a capture sphere for particles in radial motion, and more recently also for particles in non-radial motion, in which the Poynting-Robertson radiation drag efficiently removes the orbital angular momentum of the particles, reducing it to zero. Here we develop this idea further, showing that "levitation" on the Eddington sphere (above the stellar surface) is a stateof stable equilibrium, and discuss its implications for Hoyle-Lyttleton accretion onto a luminous star. When the Eddington sphere is present, the cross-section of a compact star for actual accretion is typically less than the geometrical
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy & Astrophysics
ISSN
0004-6361
e-ISSN
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Volume of the periodical
546
Issue of the periodical within the volume
OCT 2012
Country of publishing house
FR - FRANCE
Number of pages
5
Pages from-to
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UT code for WoS article
000310349100054
EID of the result in the Scopus database
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