A systematic study of the high-frequency bump in the black-hole low-mass X-ray binary GX 339-4
A systematic study of the high-frequency bump in the black-hole low-mass X-ray binary GX 339-4
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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The high-frequency bump, characterized by a frequency exceeding ~30 Hz, represents a seldom-explored time-variability feature in the power density spectrum (PDS) of black-hole X-ray binaries. In the 2002, 2004, 2007 and 2010 outbursts of GX 339-4, the bump has been occasionally observed in conjunction with type-C quasi-periodic oscillations (QPOs)....
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A systematic study of the high-frequency bump in the black-hole low-mass X-ray binary GX 339-4
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TN_cdi_proquest_journals_2892395952
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2892395952
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2331-8422
