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1997A&A...327L..33K - Astronomy and Astrophysics, volume 327, L33-35 (1997/11-3)
A possible 13.81 d period of the X-ray binary 4U 1700-377.
KOENIG M. and MAISACK M.
Abstract (from CDS):
We report the results of a temporal analysis of CGRO BATSE and RXTE ASM All-Sky monitor X-ray light curves of the high mass XRB 4U 1700-377. In addition to the known orbital period of 3.41d we found evidence for the existence of a second periodicity of about 13.81d in the light curves of both satellites. We suggest that this new period might be due to the free precession of the neutron star.
Abstract Copyright: ∼
Journal keyword(s): X-rays: stars
Simbad objects: 3
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