Spectroscopic orbit of the star HR96

Details Spectroscopic orbit of the star HR96 Spectroscopic orbit of the star HR96

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26as...53...29h&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 53, July 1983, p. 29-31.

Astronomy and Astrophysics

Astrophysics

Astrometry, B Stars, Binary Stars, Orbital Elements, Eclipsing Binary Stars, Radial Velocity

Scientific paper

The rather long orbital period of 48.2905 days and large eccentricity of
0.384, together with a mass function of 0.107, are derived for the
spectroscopic binary HR 96. The extensive photographic plate material
employed in the present study does not support previously suggested
spectroscopic and photometric peculiarities and variability.

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