Accretion discs, jets and high energy phenomena in astrophysics: Les Houches Session LXXVIII, 29 July-23 August, 2002The accretion process is thought to play a key role in the Universe. This book explains, in a form intelligible to graduate students, its relation to the formation of new ...
About this paper Cite this paper Katz, J.I. (1985). Accretion Discs. In: Lamb, D.Q., Patterson, J. (eds) Cataclysmic Variables and Low-Mass X-Ray Binaries. Astrophysics and Space Science Library, vol 113. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5319-2_44 Download ...
<italic>Context. </italic>Radiation from accretion discs in cataclysmicvariable stars (CVs) provides fundamental information about the properties of these close binary systems and about the physicsof accretion in general. Of particular interest are dwarf
Fragile, P.C., Liska, M. (2025). Tilted Accretion Disks. In: Bambi, C., Mizuno, Y., Shashank, S., Yuan, F. (eds) New Frontiers in GRMHD Simulations. Springer Series in Astrophysics and Cosmology. Springer, Singapore. https://doi.org/10.1007/978-981-97-8522-3_11 Download citation...
A photometric selection of white dwarf candidates in Sloan Digital Sky Survey Data Release 10. Mon. Not. R. Astron. Soc. 448, 2260–2274 (2015). ADS Google Scholar Horne, K. & Marsh, T. R. Emission line formation in accretion discs. Mon. Not. R. Astron. Soc. 218, 761–773 (...
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Astronomy & AstrophysicsB. Bitsch, M. Lambrechts, A. Johansen, The growth of planets by pebble accretion in evolving protoplanetary discs. Astron Astrophys 582, A112 (2015).Bitsch, B., Lambrechts, M., Johansen, A.: The growth of planets by pebble accretion in evolving protoplanetary discs...
Keywords:accretion,accretiondiscs±magnetic®elds±MHD±turbulence±stars: magnetic®elds. 1INTRODUCTION Accretiondiscsareubiquitousinastrophysicsandinparticularin accretingobjectslikecataclysmicvariables,X-raybinariesor youngstars.Formanyyearsmagnetic®eldshavebeenincluded ...
On the structure of quasi-Keplerian accretion discs surrounding millisecond X-ray pulsarsdoi:10.1007/s12036-020-09643-w97.80.Jp X-ray binaries97.60.Gb pulsars97.10.Gz accretion and accretion discsIn this study, we investigated the time-independent dynamics (disc structure, forces and torques) of ...
The resulting rotation rates are an order of magnitude lower than the values expected for direct accretion on to the stellar surface, and are consistent with observed values.A. Collier CameronC. G. CampbellH. QuaintrellAstronomy and AstrophysicsAstronomy and Astrophysics...