The Mass Ratio of the O-type Binary 15 Monocerotis

Details The Mass Ratio of the O-type Binary 15 Monocerotis The Mass Ratio of the O-type Binary 15 Monocerotis

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...19410506b&link_type=abstract

American Astronomical Society Meeting 194, #105.06

Astronomy and Astrophysics

Astronomy

Scientific paper

The bright O-type star 15 Mon is an astrometric and spectroscopic binary with a 25 year orbital period. We present radial velocity measurements from the GSU/CHARA "Multiple Telescope Telescope" (MTT), a 1-m class spectroscopic telescope. We also present updated orbital parameters, mass ratio and, using a tomography algorithm, direct spectral typing of the secondary of this interesting system.

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