The XMM-Newton survey of the Small Magellanic Cloud: XMMU J010633.1-731543 and XMMU J010743.1-715953, two new Be/X-ray binary systems★
Abstract
In the course of the XMM-Newton survey of the Small Magellanic Cloud (SMC), two new bright X-ray sources were discovered exhibiting the spectral characteristics of high-mass X-ray binaries - but revealing only weak evidence for pulsations in just one of the objects (at 153 s in XMMU J010743.1-715953). The accurate X-ray source locations permit the identification of these X-ray sources with Be stars, thereby strongly suggesting that these systems are new Be/X-ray binaries. From blue spectra the proposed classification for XMMU J010633.1-731543 is B0.5-1Ve and for XMMU J010743.1-715953 it is B2IV-Ve.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- July 2012
- DOI:
- 10.1111/j.1365-2966.2012.21193.x
- arXiv:
- arXiv:1204.5903
- Bibcode:
- 2012MNRAS.424..282C
- Keywords:
-
- stars: neutron;
- X-rays: binaries;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- MNRAS (accepted), 12 pages, 17 figures, 4 tables