Restrictions to neutron star properties based on twin-peak
quasi-periodic oscillations (Conference Paper)

D 2012

Restrictions to neutron star properties based on twin-peak quasi-periodic oscillations (Conference Paper)

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

Základní údaje

Originální název

Restrictions to neutron star properties based on twin-peak quasi-periodic oscillations (Conference Paper)

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. 319-320, 2 s. 2012

Nakladatel

Cambridge University Press

Další údaje

Jazyk

angličtina

Typ výsledku

Stať ve sborníku

Obor

10308 Astronomy

Utajení

není předmětem státního či obchodního tajemství

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/S1743921312020200

Klíčová slova anglicky

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

Štítky

FÚ, sbornik

Příznaky

Mezinárodní význam

Změněno: 27. 4. 2021 09:45, Jan Vlha

Anotace

V originále

We consider twin-peak quasi-periodic oscillations (QPOs) observed in the accreting low-mass neutron star (NS) binaries and explore restrictions to NS properties that are implied by various QPO models. For each model and each source, the consideration results in a specific relation between the NS mass M and the angular-momentum j rather than in their single preferred combination. Furthermore, the inferred restrictions on NS properties (or QPO models) are weaker for the low-frequency sources than for thehigh-frequency sources.

Citovat

BAKALA, Pavel; Kateřina GOLUCHOVÁ; Zdeněk STUCHLÍK; Eva ŠRÁMKOVÁ; Gabriel TÖRÖK a Martin URBANEC. Restrictions to neutron star properties based on twin-peak quasi-periodic oscillations (Conference Paper). In Proceedings of the International Astronomical Union. Cambridge, UK: Cambridge University Press, 2012, s. 319-320. ISBN 978-1-107-03379-5. Dostupné z: https://doi.org/10.1017/S1743921312020200.

@inproceedings{42561,
   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/S1743921312020200},
   keywords = {Stars: fundamental parameters; Stars: neutron; Stars: rotation; X-rays: binaries},
   language = {eng},
   location = {Cambridge, UK},
   isbn = {978-1-107-03379-5},
   pages = {319-320},
   publisher = {Cambridge University Press},
   title = {Restrictions to neutron star properties based on twin-peak quasi-periodic oscillations (Conference Paper)},
   year = {2012}
}

TY  - CONF
ID  - 42561
AU  - Bakala, Pavel - Goluchová, Kateřina - Stuchlík, Zdeněk - Šrámková, Eva - Török, Gabriel - Urbanec, Martin
PY  - 2012
TI  - Restrictions to neutron star properties based on twin-peak quasi-periodic oscillations (Conference Paper)
PB  - Cambridge University Press
CY  - Cambridge, UK
SN  - 9781107033795
KW  - Stars: fundamental parameters
KW  - Stars: neutron
KW  - Stars: rotation
KW  - X-rays: binaries
N2  - We consider twin-peak quasi-periodic oscillations (QPOs) observed in the accreting low-mass neutron star (NS) binaries and explore restrictions to NS properties that are implied by various QPO models. For each model and each source, the consideration results in a specific relation between the NS mass M and the angular-momentum j rather than in their single preferred combination. Furthermore, the inferred restrictions on NS properties (or QPO models) are weaker for the low-frequency sources than for thehigh-frequency sources.
ER  -

BAKALA, Pavel; Kateřina GOLUCHOVÁ; Zdeněk STUCHLÍK; Eva ŠRÁMKOVÁ; Gabriel TÖRÖK a Martin URBANEC. Restrictions to neutron star properties based on twin-peak quasi-periodic oscillations (Conference Paper). In \textit{Proceedings of the International Astronomical Union}. Cambridge, UK: Cambridge University Press, 2012, s.~319-320. ISBN~978-1-107-03379-5. Dostupné z: https://doi.org/10.1017/S1743921312020200.

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