| GOLUCHOVÁ, Kateřina, Gabriel TÖRÖK, Martin URBANEC, Gabriela URBANCOVÁ a Eva ŠRÁMKOVÁ. Innermost stable circular orbits around compact stars: Terms that are quadratic in spin. 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. 1. vyd. Opava (Česká republika): Slezská univerzita v Opavě, Filozoficko–přírodovědecká fakulta v Opavě, Ústav fyziky, 2017, s. 23-32. ISBN 978-80-7510-256-0. |
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@inproceedings{28336,
author = {Goluchová, Kateřina and Török, Gabriel and Urbanec, Martin and Urbancová, Gabriela and Šrámková, Eva},
address = {Opava (Česká republika)},
booktitle = {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},
edition = {1.},
editor = {Z. Stuchlík, G. Török a V. Karas},
keywords = {X-rays: binaries; accretion; accretion disks; stars: neutron},
howpublished = {tištěná verze "print"},
language = {eng},
location = {Opava (Česká republika)},
isbn = {978-80-7510-256-0},
pages = {23-32},
publisher = {Slezská univerzita v Opavě, Filozoficko–přírodovědecká fakulta v Opavě, Ústav fyziky},
title = {Innermost stable circular orbits around compact stars: Terms that are quadratic in spin},
url = {http://proceedings.physics.cz/index.php/ragtime-book/proceedings-of-ragtime-17-19},
year = {2017}
}
TY - JOUR
ID - 28336
AU - Goluchová, Kateřina - Török, Gabriel - Urbanec, Martin - Urbancová, Gabriela - Šrámková, Eva
PY - 2017
TI - Innermost stable circular orbits around compact stars: Terms that are quadratic in spin
PB - Slezská univerzita v Opavě, Filozoficko–přírodovědecká fakulta v Opavě, Ústav fyziky
CY - Opava (Česká republika)
SN - 9788075102560
KW - X-rays: binaries
KW - accretion
KW - accretion disks
KW - stars: neutron
UR - http://proceedings.physics.cz/index.php/ragtime-book/proceedings-of-ragtime-17-19
L2 - http://proceedings.physics.cz/index.php/ragtime-book/proceedings-of-ragtime-17-19
N2 - Orbital motion close to a rotating compact star is largely affected by strong gravity. Location of the innermost stable circular orbit (ISCO) is determined trough interplay between the effects of general relativity and the effects of Newtonian physics that are associated to oblateness of the compact star. The Keplerian frequency at this orbit may increase as well as decrease when the compact star angular momentum increases. In this context we explore behaviour of the ISCO frequency for compact star models calculated within the Hartle-Thorne spacetime approximation.
ER -
GOLUCHOVÁ, Kateřina, Gabriel TÖRÖK, Martin URBANEC, Gabriela URBANCOVÁ a Eva ŠRÁMKOVÁ. Innermost stable circular orbits around compact stars: Terms that are quadratic in spin. In Z. Stuchlík, G. Török a V. Karas. \textit{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}. 1. vyd. Opava (Česká republika): Slezská univerzita v Opavě, Filozoficko–přírodovědecká fakulta v Opavě, Ústav fyziky, 2017, s.~23-32. ISBN~978-80-7510-256-0.
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