Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-07-25
Mon.Not.Roy.Astron.Soc. 328 (2001) 139
Astronomy and Astrophysics
Astrophysics
Accepted for publication in MNRAS, 9 pages
Scientific paper
10.1046/j.1365-8711.2001.04849.x
We have studied the long term variability of LMC X-3 in optical lightcurves spanning six years, in order to search for optical signatures which could confirm/refute the suggestion that the `modulation' is the result of accretion rate variability rather than accretion disc precession. We find that there is no stable period in the optical lightcurves, that the optical and X-ray lightcurves are correlated, with an X-ray lag and that there is no modulation in the optical colours. We argue that these effects agree with the variable mass accretion rate model proposed by Wilms et al. (2001).
Brocksopp Catherine
Groot Paul J.
Wilms Joern
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