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

Organizační jednotka

Filozoficko-přírodovědecká fakulta v Opavě

ISBN

978-1-107-03379-5

ISSN

DOI

http://dx.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://dx.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 = {http://dx.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  - JOUR
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://dx.doi.org/10.1017/S1743921312020200.

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