Suzaku observations of the HMXB 1A 1118-61
Abstract
We present broad band analysis of the Be/X-ray transient 1A 1118-61 by Suzaku at the peak of its 3rd observed outburst in January 2009 and 2 weeks later when the source flux had decayed by an order of magnitude. The continuum was modeled with a \texttt{cutoffpl} model as well as a compTT model, with both cases requiring an additional black body component at lower energies. We confirm the detection of a cyclotron line at ~5 keV and discuss the possibility of a first harmonic at ~110 keV. Pulse profile comparisons show a change in the profile structure at lower energies, an indication for possible changes in the accretion geometry. Phase resolved spectroscopy in the outburst data show a change in the continuum throughout the pulse period. The decrease in the CRSF centroid energy also indicates that the viewing angle on the accretion column is changing throughout the pulse period.
Keywords
Cite
@article{arxiv.1103.1370,
title = {Suzaku observations of the HMXB 1A 1118-61},
author = {Slawomir Suchy and Katja Pottschmidt and Richard E. Rothschild and Joern Wilms and Felix Fuerst and Laura Barragan and Isabel Caballero and Victoria Grinberg and Ingo Kreykenbohm and Victor Doroshenko and Andrea Santangelo and Ruediger Staubert and Yukikatsu Terada and Wataru Iwakari and Kazuo Makishima},
journal= {arXiv preprint arXiv:1103.1370},
year = {2015}
}
Comments
accepted by ApJ