Year: 2005
Type: article
Abstract: Some of the more promising ideas about the origin of the high frequency variability (kHz QPOs) in the observed X‐ray emissions of low‐mass X‐ray binaries are contrasted with less promising ones. (© 2005 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
Source: Astronomische Nachrichten
Author: W. Kluźniak
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W2105761671
