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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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