X Persei - Optical 13.9-minute periodicity

Details X Persei - Optical 13.9-minute periodicity X Persei - Optical 13.9-minute periodicity

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..312l&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, April 1987, p. 312-320. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Optical Emission Spectroscopy, Pulsars, Stellar Spectrophotometry, Variable Stars, Visible Spectrum, X Ray Binaries, Spectrum Analysis, Ubv Spectra

Scientific paper

Broadband (B filter) optical-continuum observations of the X-ray binary
X Per during October 30 to November 1, 1985 show a variability with the
period of an X-ray pulsar. The amplitude of the variability is about 0.8
percent, the period being 13.911 + or - 0.004 min.

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