Other formats:
BibTeX
LaTeX
RIS
@inproceedings{42053, author = {Abramowicz, Marek and Stuchlík, Zdeněk and Šrámková, Eva and Török, Gabriel}, address = {Cambridge}, booktitle = {Binary Stars as Critical Tools and Tests in Contemporary Astrophysics}, doi = {http://dx.doi.org/10.1017/S1743921307006473}, keywords = {Black hole physics, X-rays: binaries}, language = {eng}, location = {Cambridge}, isbn = {978-0-521-86348-3}, pages = {119-121}, publisher = {Cambridge University Press}, title = {QPOs in microquasars: the spin problem}, year = {2006} }
TY - JOUR ID - 42053 AU - Abramowicz, Marek - Stuchlík, Zdeněk - Šrámková, Eva - Török, Gabriel PY - 2006 TI - QPOs in microquasars: the spin problem PB - Cambridge University Press CY - Cambridge SN - 9780521863483 KW - Black hole physics, X-rays: binaries N2 - In the Galactic microquasars with double peak kHz quasi-periodic oscillations (QPOs), the ratio of the two frequencies is 3:2. This supports the suggestion that double peak kHz QPOs are due to a non-linear resonance between two modes of accretion disk oscillations. For the microquasars with known mass, we briefly compare the black hole spin estimates based on the orbital resonance model with the recently reported spin predictions obtained by fitting the spectral continua. ER -
ABRAMOWICZ, Marek, Zdeněk STUCHLÍK, Eva ŠRÁMKOVÁ and Gabriel TÖRÖK. QPOs in microquasars: the spin problem. In \textit{Binary Stars as Critical Tools and Tests in Contemporary Astrophysics}. Cambridge: Cambridge University Press, 2006, p.~119-121. ISBN~978-0-521-86348-3. Available from: https://dx.doi.org/10.1017/S1743921307006473.
|