GRS 1758-258: A rare persistent hard state Black Hole
| dc.contributor.author | Obst, Maria | |
| dc.contributor.author | Pottschmidt, Katja | |
| dc.contributor.author | Lohfink, A. | |
| dc.contributor.author | Wilms, J. | |
| dc.contributor.author | Bel, M. Cadolle | |
| dc.contributor.author | Smith, D. M. | |
| dc.contributor.author | Tomsick, J. A. | |
| dc.contributor.author | Kreykenbohm, I. | |
| dc.contributor.author | Rodrigues, B. H. | |
| dc.date.accessioned | 2023-09-14T20:46:20Z | |
| dc.date.available | 2023-09-14T20:46:20Z | |
| dc.description.abstract | We present the spectral and timing evolution of GRS 1758-258, one of only three known persistent black hole binaries in our Galaxy, based on 11 years of RXTE-PCA observations. During this time, GRS 1758-258 entered a thermally dominated soft state seven times, showing a strong decline in the 3-20 keV flux rather than an increase. There is only one other source that displays this behavior. In its hardness intensity diagram below 20 keV, GRS 1758-258 shows a hysteresis of hard and soft state fluxes like transient sources in outburst, but with deviations from their typical q-tracks. The spectral flux light curve does not contain any orbital modulations in the range of 1 to 30 days, but in the dynamic power spectrum significant peaks are drifting between 18.47 ± 0.25 and 18.04 ± 0.22 days. | en |
| dc.description.sponsorship | We thank J.E. Davis for the development of the slxfig module. This work has been partly funded by the EU under contract ITN 215212 “Black Hole Universe” | en |
| dc.description.uri | https://articles.adsabs.harvard.edu/pdf/2013HEAD...1312654O | en |
| dc.format.extent | 1 page | en |
| dc.genre | posters | en |
| dc.identifier | doi:10.13016/m2nxkl-bgf1 | |
| dc.identifier.uri | http://hdl.handle.net/11603/29670 | |
| dc.language.iso | en | en |
| dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
| dc.relation.ispartof | UMBC Center for Space Sciences and Technology | |
| dc.relation.ispartof | UMBC Faculty Collection | |
| dc.relation.ispartof | UMBC Physics Department | |
| dc.rights | This 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 |
| dc.title | GRS 1758-258: A rare persistent hard state Black Hole | en |
| dc.title.alternative | GRS 1758-258: Long Term Evolution of a Rare Persistent Hard State Black Hole | en |
| dc.type | Text | en |
| dcterms.creator | https://orcid.org/0000-0002-4656-6881 | en |