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

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19240%2F12%3A%230004524" target="_blank" >RIV/47813059:19240/12:#0004524 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1017/S1743921312020200" target="_blank" >http://dx.doi.org/10.1017/S1743921312020200</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S1743921312020200" target="_blank" >10.1017/S1743921312020200</a>

Result language
angličtina
Original language name
Restrictions to neutron star properties based on twin-peak quasi-periodic oscillations (Conference Paper)
Original language description
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.
Czech name
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Czech description
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Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Proceedings of the International Astronomical Union
ISBN
978-1-107-03379-5
ISSN
1743-9213
e-ISSN
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Number of pages
2
Pages from-to
319-320
Publisher name
Cambridge University Press
Place of publication
Cambridge, UK
Event location
Peking, Čína
Event date
Aug 20, 2012
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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