State transitions and jet formation in black hole binaries

dc.contributor.authorKalemci, Emrah
dc.contributor.authorTomsick, John A.
dc.contributor.authorRothschild, Richard E.
dc.contributor.authorPottschmidt, Katja
dc.contributor.authorMigliari, Simone
dc.contributor.authorCorbel, Stephane
dc.contributor.authorKaaret, Philip
dc.date.accessioned2023-10-06T21:09:21Z
dc.date.available2023-10-06T21:09:21Z
dc.date.issued2007-08-28
dc.descriptionVI Microquasar Workshop: Microquasars and Beyond, September 18-22 2006, Società del Casino, Como, Italyen_US
dc.description.abstractThe daily monitoring observations of black hole transients with RXTE provided important clues on the conditions of the state transitions, both in terms of spectra and timing. The recent addition of monitoring in the optical-infrared and the radio band significantly extended our knowledge of the relation between the jets and the spectral states. However, there are still very important unanswered questions, most importantly, whether the formation of the jet triggers any change in the spectral and temporal properties of the source. The answer to this question is also intrinsically related to the origin of the hard X-ray emission. In this work, the relation between the jet and the state transitions is discussed, using the data from GX 339−4, 4U 1543−47, H 1743−322, and GRO J1655−40, concentrating on the evolution of spectral and temporal parameters before, during and after the formation of the jet.en_US
dc.description.sponsorshipE.K. is supported by the European Commission through a FP6 Marie-Curie International Reintegration Grant (INDAM). E.K. acknowledges partial support of TÜB˙ITAK. This project is supported by NASA Grant NNG06GB90G. EK thanks Rob Fender, Catherine Brocksopp, and Micheal Rupen for radio data, Michelle Buxton and Charles Bailyn for optical & infrared data. EK thanks the organizers of the VIth Microquasar Workshop, and Sara Markoff, Piergiorgio Casella, and Jeroen Homan for useful discussions during the meeting. R.E.R and K.P acknowledge NASA support NAS5-30720.en_US
dc.description.urihttps://pos.sissa.it/033/012en_US
dc.format.extent11 pagesen_US
dc.genreconference papers and proceedingsen_US
dc.identifierdoi:10.13016/m2urmd-jjxo
dc.identifier.citationKalemci, Emrah, John Tomsick, Richard E. Rothschild, Katja Pottschmidt, Simone Migliari, Stephane Corbel, and Philip Kaaret. “State Transitions and Jet Formation in Black Hole Binaries.” In Proceedings of VI Microquasar Workshop: Microquasars and Beyond — PoS(MQW6), 33:012. SISSA Medialab, 2007. https://doi.org/10.22323/1.033.0012.en_US
dc.identifier.urihttps://doi.org/10.22323/1.033.0012
dc.identifier.urihttp://hdl.handle.net/11603/30026
dc.language.isoen_USen_US
dc.publisherProceedings of Scienceen_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.rightsAttribution-NonCommercial-ShareAlike 1.0 Generic (CC BY-NC-SA 1.0)*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-sa/1.0/*
dc.titleState transitions and jet formation in black hole binariesen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-4656-6881en_US

Files

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
MQW6_012.pdf
Size:
368.36 KB
Format:
Adobe Portable Document Format
Description:

License bundle

Now showing 1 - 1 of 1
No Thumbnail Available
Name:
license.txt
Size:
2.56 KB
Format:
Item-specific license agreed upon to submission
Description: