D
2017
The study on behaviour of thin accretion disc affected by Poynting–Robertson effect
LANČOVÁ, Debora; Pavel BAKALA; Kateřina GOLUCHOVÁ; Maurizio FALANGA; Vittorio DE FALCO et. al.
Basic information
Original name
The study on behaviour of thin accretion disc affected by Poynting–Robertson effect
Authors
LANČOVÁ, Debora; Pavel BAKALA; Kateřina GOLUCHOVÁ; Maurizio FALANGA; Vittorio DE FALCO and Luigi STELLA
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
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"
RIV identification code
RIV/47813059:19240/17:A0000002
Organization
Filozoficko-přírodovědecká fakulta – Slezská univerzita v Opavě – Repository
EID Scopus
2-s2.0-85041833355
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.
In the original language
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.
Displayed: 21/12/2025 18:27