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@article{43860,
author = {Bakala, Pavel and Stuchlík, Zdeněk and Török, Gabriel},
article_location = {DE - Spolková republika Německo},
article_number = {4},
doi = {http://dx.doi.org/10.2478/s11534-007-0039-0},
keywords = {X-rays, binaries, accretion, accretion discs, stars, neutron},
language = {eng},
issn = {1895-1082},
journal = {CENTRAL EUROPEAN JOURNAL OF PHYSICS},
title = {A remark about possible unity of the neutron star and black hole high frequency QPOs},
volume = {5},
year = {2007}
}
TY - JOUR
ID - 43860
AU - Bakala, Pavel - Stuchlík, Zdeněk - Török, Gabriel
PY - 2007
TI - A remark about possible unity of the neutron star and black hole high frequency QPOs
JF - CENTRAL EUROPEAN JOURNAL OF PHYSICS
VL - 5
IS - 4
SP - 457-462
EP - 457-462
SN - 18951082
KW - X-rays, binaries, accretion, accretion discs, stars, neutron
N2 - Series of papers discuss on the basis of phenomenological arguments whether the high frequency quasiperiodic oscillations (kHz QPOs) observed in the neutron-star and black-hole X-ray sources originate in the same physical mechanism. Recently it was suggested that a general trend seen in neutron star kHz QPOs rather exclude such a uniform origin. On the example of the atoll source 4U 1636-53 we illustrate that this is not neccesarily true.
ER -
BAKALA, Pavel, Zdeněk STUCHLÍK and Gabriel TÖRÖK. A remark about possible unity of the neutron star and black hole high frequency QPOs. \textit{CENTRAL EUROPEAN JOURNAL OF PHYSICS}. DE - Spolková republika Německo, 2007, vol.~5, No~4, p.~457-462. ISSN~1895-1082. Available from: https://dx.doi.org/10.2478/s11534-007-0039-0.
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