A search for X-ray periodicities from 4U 1700-37

Details A search for X-ray periodicities from 4U 1700-37 A search for X-ray periodicities from 4U 1700-37

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.222p..21g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 222, Oct. 1, 1986, p. 21P-25P.

Astronomy and Astrophysics

Astronomy

24

Binary Stars, Periodic Variations, Spaceborne Astronomy, Stellar Spectrophotometry, X Ray Spectra, Exosat Satellite, Orbital Elements

Scientific paper

Using the EXOSAT observatory the authors have observed the massive X-ray binary system 4U 1700-37 for more than one complete orbital period. The authors report on a search for X-ray pulsations. No coherent periodicity was detected with upper limits to the pulsed fraction over the frequency range 256 to 2×10-5Hz (corresponding to rotational periods of 3.9 ms to 50000 s) of ≡0.5 to ≡50 per cent.

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