The Orbit of the Spectroscopic Binary phi Aquilae

Details The Orbit of the Spectroscopic Binary phi Aquilae The Orbit of the Spectroscopic Binary phi Aquilae

Dec 1922

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1922pdao....2..179h&link_type=abstract

Publications of the Dominion Observatory Ottawa, vol. 2, pp.179-182

Physics

Scientific paper

Seventeen single-prism spectrograms of the star phi Aquilae form the
basis of the determination of its spectroscopic orbit. Its type is A2
and its spectrum contains several lines suitable for measurement, the
probable error of a plate being /-1.6 km. per sec. The period is 3.3204
days and eccentricity .055.

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