Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2012-04-26
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
MNRAS (accepted), 12 pages, 17 figures, 4 tables
Scientific paper
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 characteris- tics of High Mass X-ray Binaries - but revealing only weak evidence for pulsations in just one of the objects(at 153s in XMMUJ010743.1-715953). The accurate X- ray source locations permit the identi?cation of these X-ray source with Be stars, thereby strongly suggesting these systems are new Be/X-ray binaries. From blue spectra the proposed classi?cation for XMMUJ010633.1-731543 is B0.5-1Ve and for XMMUJ010743.1-715953 it is B2IV-Ve.
Bartlett E. S.
Coe Malcolm J.
Filipović Miroslav
Haberl Franck
Hatzidimitriou Despina
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