A spectroscopic study of the binary system beta ARIETIS

Details A spectroscopic study of the binary system beta ARIETIS A spectroscopic study of the binary system beta ARIETIS

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988obs...108..228h&link_type=abstract

The Observatory, vol. 108, p. 228-232 (1988)

Physics

2

Scientific paper

Radial velocities derived from 70 spectrograms of the binary system β Arietis are presented. The resultant orbit of high eccentricity (e = 0.89) is in excellent agreement with previous studies. The short-period (≅0.05 day) variations in radial velocity reported by Barbano di Belgioso et al. and attributed by them to pulsational instability are not confirmed by these data.

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