Suchy S, Pottschmidt K, Rothschild RE, Wilms J, Fürst F, Barragan L, Caballero I, Grinberg V, Kreykenbohm I, Doroshenko V, Santangelo A, Staubert R, Terada Y, Iwakari W, Makishima K (2011)
Publication Status: Published
Publication Type: Journal article
Publication year: 2011
Publisher: IOP PUBLISHING LTD
Book Volume: 733
Article Number: ARTN 15
Journal Issue: 1
DOI: 10.1088/0004-637X/733/1/15
We present broadband analysis of the Be/X-ray transient 1A 1118-61 by Suzaku at the peak of its third observed outburst in 2009 January and two weeks later when the source flux had decayed by an order of magnitude. The continuum was modeled with a cutoffpl model as well as a compTT model, with both cases requiring an additional blackbody component at lower energies. We confirm the detection of a cyclotron line at similar to 55 keV and discuss the possibility of a first harmonic at similar to 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 shows a change in the continuum throughout the pulse period. The decrease in the cyclotron resonance scattering feature centroid energy also indicates that the viewing angle on the accretion column is changing throughout the pulse period.
APA:
Suchy, S., Pottschmidt, K., Rothschild, R.E., Wilms, J., Fürst, F., Barragan, L.,... Makishima, K. (2011). SUZAKU OBSERVATIONS OF THE HMXB 1A 1118-61. Astrophysical Journal, 733(1). https://doi.org/10.1088/0004-637X/733/1/15
MLA:
Suchy, Slawomir, et al. "SUZAKU OBSERVATIONS OF THE HMXB 1A 1118-61." Astrophysical Journal 733.1 (2011).
BibTeX: Download