A possible 13.81 D period of the X-ray binary 4U 1700-377

Details A possible 13.81 D period of the X-ray binary 4U 1700-377 A possible 13.81 D period of the X-ray binary 4U 1700-377

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...327l..33k&link_type=abstract

Astronomy and Astrophysics, v.327, p.L33-L35 (1997)

Astronomy and Astrophysics

Astrophysics

5

X-Rays: Stars

Scientific paper

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 3.41 d we found evidence for the existence of a second periodicity of about 13.81 d in the light curves of both satellites. We suggest that this new period might be due to the free precession of the neutron star.

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