NuSTAR detection of 4s Hard X-ray Lags from the Accreting Pulsar GS 0834-430

NuSTAR detection of 4s Hard X-ray Lags from the Accreting Pulsar GS 0834-430

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The NuSTAR hard X-ray telescope observed the transient Be/X-ray binary GS 0834-430 during its 2012 outburst. The source is detected between 3 - 79 keV with high statistical significance, and we were able to perform very accurate spectral and timing analysis. The phase-averaged spectrum is consistent...

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Main Authors: Bachetti, Matteo (Author), Miyasaka, Hiromasa (Author), Harrison, Fiona A. (Author), Furst, Felix (Author), Barret, Didier (Author), Bellm, Eric C. (Author), Boggs, Steven E. (Author), Chakrabarty, Deepto (Contributor), Chenevez, Jerome (Author), Christensen, Finn E. (Author), Craig, William W. (Author), Grefenstette, Brian W. (Author), Hailey, Charles J. (Author), Madsen, Kristin K. (Author), Natalucci, Lorenzo (Author), Pottschmidt, Katja (Author), Stern, Daniel (Author), Tomsick, John A. (Author), Walton, Dominic J. (Author), Wilms, Jörn (Author), Zhang, William (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: EDP Sciences, 2014-09-09T13:15:05Z.
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