State transition of the new black hole transient XTE J1650–500

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dc.contributor.authorKalemci, E.
dc.contributor.authorTomsick, J.A.
dc.contributor.authorRothschild, R.A.
dc.contributor.authorPottschmidt, Katja
dc.contributor.authorKaaret, P.
dc.contributor.authorWijnands, R.
dc.contributor.authorMiller, J. M.
dc.date.accessioned2023-10-12T19:20:57Z
dc.date.available2023-10-12T19:20:57Z
dc.date.issued2002-02-25
dc.description.abstractWe present results on the temporal properties of the state transition from the soft to hard state in the new black hole transient XTE J1650–500. After MJD 52232, the power law index hardened, rms amplitude of the power spectrum increased significantly, and QPOs were observed. We also found enhanced lags during the transition as observed in Cyg X-1. The enhanced lags may be due to the presence of a larger Comptonizing area of the base of a jet, but another possibility is also discussed. We also show the correlation between the peak frequencies of the fit components, which is consistent with previous reports of such correlations for various kinds of X-ray binaries.
dc.description.urihttps://online.kitp.ucsb.edu/online/bhole-c02/p_kalemci/en_US
dc.format.extent1 pageen_US
dc.genrepostersen_US
dc.identifierdoi:10.13016/m2sqxk-wjrz
dc.identifier.urihttp://hdl.handle.net/11603/30119
dc.language.isoen_USen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Physics Department
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.en_US
dc.titleState transition of the new black hole transient XTE J1650–500en_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-4656-6881en_US

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