Radiative Corrections to the Neutron Star Mass Inferred from QPO Frequencies

@article{43582,
   author = {Abramowicz, Marek},
   article_location = {PL - Polská republika},
   article_number = {4},
   keywords = {QUASI-PERIODIC OSCILLATIONS, X-RAY BINARIES, CYGNUS X-2, 4U 1608-52, DEPENDENCE},
   language = {eng},
   issn = {0001-5237},
   journal = {Acta Astronomica},
   title = {Radiative Corrections to the Neutron Star Mass Inferred from QPO Frequencies},
   volume = {61},
   year = {2011}
}

TY  - JOUR
ID  - 43582
AU  - Abramowicz, Marek
PY  - 2011
TI  - Radiative Corrections to the Neutron Star Mass Inferred from QPO Frequencies
JF  - Acta Astronomica
VL  - 61
IS  - 4
SP  - 319-324
EP  - 319-324
SN  - 00015237
KW  - QUASI-PERIODIC OSCILLATIONS, X-RAY BINARIES, CYGNUS X-2, 4U 1608-52, DEPENDENCE
N2  - The frequencies of kHz QPOs are widely interpreted as being indicative of the values of characteristic frequencies related to orbital motion around neutron stars, e.g., the radial cpicyclic frequency. In regions directly exposed to the radiation from theluminous neutron star these frequencies change with the luminosity. Including radiative corrections will change the neutron star mass value inferred from the QPO frequencies. Radiative forces may also be behind the puzzling phenomenon of parallel tracks.
ER  - 

ABRAMOWICZ, Marek. Radiative Corrections to the Neutron Star Mass Inferred from QPO Frequencies. \textit{Acta Astronomica}. PL - Polská republika, 2011, vol.~61, No~4, p.~319-324, 5 pp. ISSN~0001-5237.