A CLUMPY STELLAR WIND AND LUMINOSITY-DEPENDENT CYCLOTRON LINE REVEALED BY THE FIRST SUZAKU OBSERVATION OF THE HIGH-MASS X-RAY BINARY 4U 1538−522
dc.contributor.author | Hemphill, Paul B. | |
dc.contributor.author | Rothschild, Richard E. | |
dc.contributor.author | Markowitz, Alex | |
dc.contributor.author | Fürst, Felix | |
dc.contributor.author | Pottschmidt, Katja | |
dc.contributor.author | Wilms, Jörn | |
dc.date.accessioned | 2023-09-06T14:33:37Z | |
dc.date.available | 2023-09-06T14:33:37Z | |
dc.date.issued | 2014-08-08 | |
dc.description.abstract | We present results from the first Suzaku observation of the high-mass X-ray binary 4U 1538−522. The broadband spectral coverage of Suzaku allows for a detailed spectral analysis, characterizing the cyclotron resonance scattering feature at 23.0 ± 0.4 keV and the iron Kα line at 6.426 ± 0.008 keV, as well as placing limits on the strengths of the iron Kβ line and the iron K edge. We track the evolution of the spectral parameters both in time and in luminosity, notably finding a significant positive correlation between cyclotron line energy and luminosity. A dip and spike in the light curve is shown to be associated with an order-of-magnitude increase in column density along the line of sight, as well as significant variation in the underlying continuum, implying the accretion of a overdense region of a clumpy stellar wind. We also present a phase-resolved analysis, with most spectral parameters of interest showing significant variation with phase. Notably, both the cyclotron line energy and the iron Kα line intensity vary significantly with phase, with the iron line intensity significantly out of phase with the pulse profile. We discuss the implications of these findings in the context of recent work in the areas of accretion column physics and cyclotron resonance scattering feature formation. | en_US |
dc.description.sponsorship | This research has made use of data and software obtained from NASA's High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Goddard Space Flight Center and the Smithsonian Astrophysical Observatory. P.B.H. was supported by NASA grant NNX13AE68G. | en_US |
dc.description.uri | https://iopscience.iop.org/article/10.1088/0004-637X/792/1/14 | en_US |
dc.format.extent | 15 pages | en_US |
dc.genre | journal articles | en_US |
dc.identifier | doi:10.13016/m2vqsr-3oxh | |
dc.identifier.citation | Hemphill, Paul B., Richard E. Rothschild, Alex Markowitz, Felix Fürst, Katja Pottschmidt, and Jörn Wilms. “A CLUMPY S℡LAR WIND AND LUMINOSITY-DEPENDENT CYCLOTRON LINE REVEALED BY THE FIRST SUZAKU OBSERVATION OF THE HIGH-MASS X-RAY BINARY 4U 1538−522.” The Astrophysical Journal 792, no. 1 (August 2014): 14. https://doi.org/10.1088/0004-637X/792/1/14. | en_US |
dc.identifier.uri | https://doi.org/10.1088/0004-637X/792/1/14 | |
dc.identifier.uri | http://hdl.handle.net/11603/29580 | |
dc.language.iso | en_US | en_US |
dc.publisher | IOP Publishing | en_US |
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_US |
dc.title | A CLUMPY STELLAR WIND AND LUMINOSITY-DEPENDENT CYCLOTRON LINE REVEALED BY THE FIRST SUZAKU OBSERVATION OF THE HIGH-MASS X-RAY BINARY 4U 1538−522 | en_US |
dc.type | Text | en_US |
dcterms.creator | https://orcid.org/0000-0002-4656-6881 | en_US |