The radial velocity and binarity of X Persei

Details The radial velocity and binarity of X Persei The radial velocity and binarity of X Persei

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.257p..21s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 257, no. 1, July 1, 1992, p. 21P-23P.

Astronomy and Astrophysics

Astronomy

5

Binary Stars, O Stars, Radial Velocity, X Ray Sources, High Resolution, Iue, Stellar Models, Stellar Spectra, Stellar Spectrophotometry

Scientific paper

It is shown on the basis of radial velocity measurements on
high-resolution spectra of X Persei from the IUE archive that there is
no variation above the level of a few km/s and thus no need for a
massive unseen component in the system. This does not rule out a neutron
star or white dwarf orbiting in the variable wind of the Be star.

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