تقرير
Broadband spectral analysis of MXB 1659-298 in its soft and hard state
| العنوان: | Broadband spectral analysis of MXB 1659-298 in its soft and hard state |
|---|---|
| المؤلفون: | Mazzola, S. M., Iaria, R., Gambino, A. F., Marino, A., Di Salvo, T., Bassi, T., Sanna, A., Riggio, A., Burderi, L. |
| سنة النشر: | 2019 |
| المجموعة: | Astrophysics |
| مصطلحات موضوعية: | Astrophysics - High Energy Astrophysical Phenomena |
| الوصف: | The X-ray transient eclipsing source MXB 1659-298 went in outburst in 1999 and 2015, respectively, during which it was observed by XMM-Newton, NuSTAR and Swift. Using these observations we studied the broadband spectrum of the source to constrain the continuum components and to verify the presence of a reflection component. We analysed the soft and hard state of the source, finding that the soft state can be modelled with a thermal component associated with the inner accretion disc plus a Comptonised component. A smeared reflection component and the presence of an ionised absorber are also requested in the best-fit model. On the other hand, the direct continuum emission in the hard state can be described by a Comptonised component with a temperature larger than 150 keV. Also in this case a reflection component and a ionised absorber are observed. Comment: Proceedings of the 12th INTEGRAL conference and 1st AHEAD Gamma-ray Workshop, Geneva (Switzerland), 11-15 February 2019, Ed. C. Ferrigno, E. Bozzo, P. von Balmoos; 4 pages, 1 figure, 2 tables, submitted to Mem. S.A.It |
| نوع الوثيقة: | Working Paper |
| URL الوصول: | http://arxiv.org/abs/1906.10960 |
| رقم الأكسشن: | edsarx.1906.10960 |
| قاعدة البيانات: | arXiv |
| الوصف غير متاح. |