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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★.

Authors :
Coe, M. J.
Haberl, F.
Sturm, R.
Bartlett, E. S.
Hatzidimitriou, D.
Townsend, L. J.
Udalski, A.
Mereghetti, S.
Filipović, M.
Source :
Monthly Notices of the Royal Astronomical Society; Jul2012, Vol. 424 Issue 1, p282-292, 11p
Publication Year :
2012

Abstract

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. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00358711
Volume :
424
Issue :
1
Database :
Complementary Index
Journal :
Monthly Notices of the Royal Astronomical Society
Publication Type :
Academic Journal
Accession number :
77509643
Full Text :
https://doi.org/10.1111/j.1365-2966.2012.21193.x