Reversal of the amplitude difference of kHz QPOs in six atoll sources

@article{42095,
   author = {Török, Gabriel},
   article_location = {FR - Francouzská republika},
   article_number = {3},
   doi = {http://dx.doi.org/10.1051/0004-6361/20079026},
   keywords = {X-rays:binaries ?Stars:neutron? Accretion, accretion disks},
   language = {eng},
   issn = {1432-0746},
   journal = {Astronomy & Astrophysics},
   title = {Reversal of the amplitude difference of kHz QPOs in six atoll sources},
   volume = {457},
   year = {2009}
}

TY  - JOUR
ID  - 42095
AU  - Török, Gabriel
PY  - 2009
TI  - Reversal of the amplitude difference of kHz QPOs in six atoll sources
JF  - Astronomy & Astrophysics
VL  - 457
IS  - 3
SP  - 661-665
EP  - 661-665
SN  - 14320746
KW  - X-rays:binaries ?Stars:neutron? Accretion, accretion disks
N2  - AIMS: For six neutron-star atoll sources (4U 1608-52, 4U 1636-53, 4U 0614+09, 4U 1728-34, 4U 1820-30 and 4U 1735-44) we investigate the relationship between the observed fractional rms amplitudes of the twin kHz QPOs. We discuss whether this displays features that could have a physical meaning in terms of the proposed QPO models. METHOD: We consider the difference in rms amplitude between the upper and lower kHz QPOs, as a function of the frequency ratio R. We compare two data sets. Set I is a collection taken from published data. Set II has rms amplitude values obtained by automatic fitting of continuous segments of RXTE-PCA observations.
ER  - 

TÖRÖK, Gabriel. Reversal of the amplitude difference of kHz QPOs in six atoll sources. \textit{Astronomy \&{} Astrophysics}. FR - Francouzská republika, 2009, vol.~457, No~3, p.~661-665. ISSN~1432-0746. Available from: https://dx.doi.org/10.1051/0004-6361/20079026.