A remark about possible unity of the neutron star and black hole high frequency QPOs

@article{41413,
   author = {Török, Gabriel and Stuchlík, Zdeněk and Bakala, Pavel},
   article_location = {WARSAW 41},
   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  - 41413
AU  - Török, Gabriel - Stuchlík, Zdeněk - Bakala, Pavel
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
PB  - VERSITA
SN  - 18951082
KW  - X-rays
KW  - binaries
KW  - accretion
KW  - accretion discs
KW  - stars
KW  - neutron
N2  - In a series of papers it was discussed, 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 instead excludes such a uniform origin. Using the example of the atoll source 4U 1636-53 we illustrate that this is not neccesarily true. (C) Versita Warsaw and Springer-Verlag Berlin Heidelberg. All rights reserved.
ER  - 

TÖRÖK, Gabriel, Zdeněk STUCHLÍK a Pavel BAKALA. A remark about possible unity of the neutron star and black hole high frequency QPOs. Online. \textit{CENTRAL EUROPEAN JOURNAL OF PHYSICS}. WARSAW 41: VERSITA, 2007, roč.~5, č.~4, s.~457-462. ISSN~1895-1082. Dostupné z: https://dx.doi.org/10.2478/s11534-007-0039-0. [citováno 2024-04-23]