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 (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

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.