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

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"

References:

RIV identification code

RIV/47813059:19240/17:A0000002

Organization

Filozoficko-přírodovědecká fakulta – Slezská univerzita v Opavě – Repository

ISBN

978-80-7510-256-0

ISSN

EID Scopus

2-s2.0-85041833355

Keywords in English

dust accretion disc; radiation; neutron stars; black holes

Tags

Tags

International impact, Reviewed

Links

GA17-16287S, research and development project.
Changed: 6/4/2018 09:21, Jan Hladík

Abstract

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.