The Spectrographic Binary HD16219

Details The Spectrographic Binary HD16219 The Spectrographic Binary HD16219

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26as...44...59h&link_type=abstract

Astronomy and Astrophysics Supplement, Vol. 44, P. 59, 1981

Astronomy and Astrophysics

Astrophysics

Scientific paper

Orbital elements are found for the late B-type spectrographic binary HD
16219. Assuming synchronous rotation and adopting a value of 35 km
s-1 for the projected equatorial rotational velocity, a
physical model of the system is developed. The system is detached and
unevolved, and no eclipses can occur.

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