HR3626 - Double-Line Spectroscopic Binary

Details HR3626 - Double-Line Spectroscopic Binary HR3626 - Double-Line Spectroscopic Binary

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pasp...94..356b&link_type=abstract

Publications of the Astronomical Society of the Pacific, Vol. 94, P. 356, 1982

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Orbital elements are determined for the double-lined spectroscopic binary HR 3626, which had previously been recognized as being only a single-lined system. A mass ratio of 1.26 + 0.02 is determined, and a magnitude difference ΔmB = 1.0 ± 0.2 is inferred from the photoelectric radial velocity dips. This leads to the conclusion that the system consists of a pair of G dwarf or subgiant stars.

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