Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-10-04
Mon.Not.Roy.Astron.Soc. 356 (2005) 502-514
Astronomy and Astrophysics
Astrophysics
15 pages, 11 figures, accepted for publication in MNRAS. A gzipped PS version of this paper with higher resolution figures is
Scientific paper
10.1111/j.1365-2966.2004.08467.x
This work represent the first major study of the optical and IR characteristics of the mass donor companions to the X-ray pulsars in the Small Magellanic Cloud (SMC). In this work several new counterparts have been identified, and possible ones confirmed, as companions to X-ray pulsars in the SMC giving a total of 34 such objects now identified. In addition this work presents three new binary periods and confirms two X-ray periods using optical data for objects in this group. This homogeneous sample has been studied as a group to determine important general characteristics that may offer insight into the evolution of such systems. In particular, the spectral class distribution shows a much greater agreement with those of isolated Be stars, and appears to be in some disagreement with the galactic population of Be stars in Be/X-ray binaries. Studies of the long term optical modulation of the Be star companions reveal an extremely variable group of objects, a fact which will almost certainly make a major contribution to the pronounced X-ray variability. The spatial distribution of these systems within the SMC is investigated and strongly suggests a link between massive star formation and the HI density distribution. Finally, studies of the circumstellar disk characteristics reveal a strong link with optical variability offering important clues into the long-term stability of such disks.
Coe Malcolm J.
Edge W. R. T.
Galache Jose Louis
McBride Vanessa A.
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