TÖRÖK, Gabriel. 3:2? In COOL DISCS, HOT FLOWS: THE VARYING FACES OF ACCRETING COMPACT OBJECTS. Sweden: Wenner Gren Fdn; Swedish Res Council; Stockholm Univ, 2008, p. 117-122. ISBN 978-0-7354-0584-4.
Other formats:   BibTeX LaTeX RIS
Basic information
Original name 3:2?
Name (in English) 3:2?
Authors TÖRÖK, Gabriel.
Edition Sweden, COOL DISCS, HOT FLOWS: THE VARYING FACES OF ACCRETING COMPACT OBJECTS, p. 117-122, 6 pp. 2008.
Publisher Wenner Gren Fdn; Swedish Res Council; Stockholm Univ
Other information
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Confidentiality degree is not subject to a state or trade secret
Organization unit Institute of physics in Opava
ISBN 978-0-7354-0584-4
ISSN 0094-243X
UT WoS 000260484300012
Keywords in English X-rays binaries, neutron stars, accretion, observation, theory
Tags FÚ, MSM4781305903, sbornik
Tags International impact
Links MSM4781305903, plan (intention).
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 6/4/2021 13:39.
Abstract
Quasiperiodic oscillations (QPOs) are observed in various neutron star (NS) and black hole (BH) X-ray binaries. It has been discussed in a serie of papers whether the 3:2 (and other) ratios pop up also in these variable frequencies of NS systems or not.Here we present a brief overview of the "3:2 subject" and summarize several recent findings of different autors which partially resolve this question. Finally, we specify some consequences for orbital QPO models.
Abstract (in English)
Quasiperiodic oscillations (QPOs) are observed in various neutron star (NS) and black hole (BH) X-ray binaries. It has been discussed in a serie of papers whether the 3:2 (and other) ratios pop up also in these variable frequencies of NS systems or not.Here we present a brief overview of the "3:2 subject" and summarize several recent findings of different autors which partially resolve this question. Finally, we specify some consequences for orbital QPO models.
PrintDisplayed: 21/5/2024 07:47