ABRAMOWICZ, Marek and A. STAH. Eddington capture sphere around luminous stars. Astronomy & Astrophysics. FR - Francouzská republika, 2012. ISSN 0004-6361. Available from: https://dx.doi.org/10.1051/0004-6361/201220187.
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Basic information
Original name Eddington capture sphere around luminous stars
Authors ABRAMOWICZ, Marek and A. STAH.
Edition Astronomy & Astrophysics, FR - Francouzská republika, 2012, 0004-6361.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
WWW www
Organization unit Faculty of Philosophy and Science in Opava
Doi http://dx.doi.org/10.1051/0004-6361/201220187
UT WoS 000310349100054
Keywords in English Accretion; Accretion disks; Stars: neutron; Radiation mechanisms: general; Relativistic processes
Tags UF
Tags International impact, Reviewed
Links MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 8/12/2020 12:20.
Abstract
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
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