LANČOVÁ, Debora, Pavel BAKALA, Kateřina GOLUCHOVÁ, Maurizio FALANGA, Vittorio DE FALCO and Luigi STELLA. The study on behaviour of thin accretion disc affected by Poynting–Robertson effect. In Z. Stuchlík, G. Török a V. Karas. Proceedings of RAGtime 17–19: Workshops on black holes and neutron stars, 17–19/23–26 Oct., 1–5 Nov. 2015/2016/2017, Opava, Czech Republic. 1st ed. Opava (Česká republika): Slezská univerzita v Opavě, Filozoficko–přírodovědecká fakulta v Opavě, Ústav fyziky, 2017, p. 127-136. ISBN 978-80-7510-256-0.
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Basic information
Original name The study on behaviour of thin accretion disc affected by Poynting–Robertson effect
Authors LANČOVÁ, Debora (203 Czech Republic, guarantor, belonging to the institution), Pavel BAKALA (203 Czech Republic, belonging to the institution), Kateřina GOLUCHOVÁ (203 Czech Republic, belonging to the institution), Maurizio FALANGA (756 Switzerland), Vittorio DE FALCO (380 Italy) and Luigi STELLA (380 Italy).
Edition 1. vyd. Opava (Česká republika), Proceedings of RAGtime 17–19: Workshops on black holes and neutron stars, 17–19/23–26 Oct., 1–5 Nov. 2015/2016/2017, Opava, Czech Republic, p. 127-136, 10 pp. 2017.
Publisher Slezská univerzita v Opavě, Filozoficko–přírodovědecká fakulta v Opavě, Ústav fyziky
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher Czech Republic
Confidentiality degree is not subject to a state or trade secret
Publication form printed version "print"
WWW RAGtime 17-19
RIV identification code RIV/47813059:19240/17:A0000002
Organization Filozoficko-přírodovědecká fakulta – Slezská univerzita v Opavě – Repository
ISBN 978-80-7510-256-0
ISSN 2336-5668
Keywords in English dust accretion disc; radiation; neutron stars; black holes
Tags 03788-2017-RRC, ASTROCOMP, GA17-16287S, IGS-1-2017, IGS12017, LM2015042, LM2015085, RAGtime 17-19, SGS-15-2016, SGS152016, ÚF
Tags International impact, Reviewed
Links GA17-16287S, research and development project.
Changed by Changed by: Jan Hladík, učo 1305. Changed: 6/4/2018 09:21.
Abstract
This study deals with the structure of a thin accretion disc under the influence of radiation pressure and Poynting-Roberson effect. The disc is approximated by inhomogeneous dust consisting of point-like particles in vicinity of a point-like source of radiation. We have developed code PR Trajectories which computes trajectories of millions of particles forming an accretion disc and provides a lot of informations about the accretion disc.
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