Restrictions to neutron star models based on twin-peak
quasi-periodic oscillations

D 2013

Restrictions to neutron star models based on twin-peak quasi-periodic oscillations

BAKALA, Pavel; Kateřina GOLUCHOVÁ; Zdeněk STUCHLÍK; Eva ŠRÁMKOVÁ; Gabriel TÖRÖK et al.

Základní údaje

Originální název

Restrictions to neutron star models based on twin-peak quasi-periodic oscillations

Autoři

BAKALA, Pavel; Kateřina GOLUCHOVÁ; Zdeněk STUCHLÍK; Eva ŠRÁMKOVÁ; Gabriel TÖRÖK a Martin URBANEC

Vydání

Cambridge, UK, Proceedings of the International Astronomical Union, od s. 524-526, 3 s. 2013

Nakladatel

Cambridge University Press

Další údaje

Jazyk

angličtina

Typ výsledku

Stať ve sborníku

Obor

10308 Astronomy

Utajení

není předmětem státního či obchodního tajemství

Odkazy

www

Označené pro přenos do RIV

Organizační jednotka

Filozoficko-přírodovědecká fakulta v Opavě

ISBN

978-1-107-03379-5

ISSN

DOI

https://doi.org/10.1017/S174392131202474X

Klíčová slova anglicky

X-rays: binaries; stars: neutron; stars: fundamental parameters; stars: rotation

Štítky

sbornik, UF

Příznaky

Mezinárodní význam

Návaznosti

GA202/09/0772, projekt VaV.

Změněno: 27. 4. 2021 09:44, Jan Vlha

Anotace

V originále

In a series of works - Török et al. (2010, 2012a) and Urbanec et al. (2010a) - we explored restrictions to neutron star properties that are implied by various models of twin-peak quasi-periodic oscillations. Here we sketch an attempt to confront the obtained mass-angular-momentum relations and limits on neutron star compactness with the parameters estimated by assuming various equations of state and the spin frequency of the atoll source 4U 1636-53.

Citovat

BAKALA, Pavel; Kateřina GOLUCHOVÁ; Zdeněk STUCHLÍK; Eva ŠRÁMKOVÁ; Gabriel TÖRÖK a Martin URBANEC. Restrictions to neutron star models based on twin-peak quasi-periodic oscillations. In Proceedings of the International Astronomical Union. Cambridge, UK: Cambridge University Press, 2013, s. 524-526. ISBN 978-1-107-03379-5. Dostupné z: https://doi.org/10.1017/S174392131202474X.

@inproceedings{43069,
   author = {Bakala, Pavel and Goluchová, Kateřina and Stuchlík, Zdeněk and Šrámková, Eva and Török, Gabriel and Urbanec, Martin},
   address = {Cambridge, UK},
   booktitle = {Proceedings of the International Astronomical Union},
   doi = {https://doi.org/10.1017/S174392131202474X},
   keywords = {X-rays: binaries; stars: neutron; stars: fundamental parameters; stars: rotation},
   language = {eng},
   location = {Cambridge, UK},
   isbn = {978-1-107-03379-5},
   pages = {524-526},
   publisher = {Cambridge University Press},
   title = {Restrictions to neutron star models based on twin-peak quasi-periodic oscillations},
   url = {http://arxiv.org/abs/1212.6670},
   year = {2013}
}

TY  - CONF
ID  - 43069
AU  - Bakala, Pavel - Goluchová, Kateřina - Stuchlík, Zdeněk - Šrámková, Eva - Török, Gabriel - Urbanec, Martin
PY  - 2013
TI  - Restrictions to neutron star models based on twin-peak quasi-periodic oscillations
PB  - Cambridge University Press
CY  - Cambridge, UK
SN  - 9781107033795
KW  - X-rays: binaries
KW  - stars: neutron
KW  - stars: fundamental parameters
KW  - stars: rotation
UR  - http://arxiv.org/abs/1212.6670
N2  - In a series of works - Török et al. (2010, 2012a) and Urbanec et al. (2010a) - we explored restrictions to neutron star properties that are implied by various models of twin-peak quasi-periodic oscillations. Here we sketch an attempt to confront the obtained mass-angular-momentum relations and limits on neutron star compactness with the parameters estimated by assuming various equations of state and the spin frequency of the atoll source 4U 1636-53.
ER  -

BAKALA, Pavel; Kateřina GOLUCHOVÁ; Zdeněk STUCHLÍK; Eva ŠRÁMKOVÁ; Gabriel TÖRÖK a Martin URBANEC. Restrictions to neutron star models based on twin-peak quasi-periodic oscillations. In \textit{Proceedings of the International Astronomical Union}. Cambridge, UK: Cambridge University Press, 2013, s.~524-526. ISBN~978-1-107-03379-5. Dostupné z: https://doi.org/10.1017/S174392131202474X.

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