The old nova BT Monocerotis

Details The old nova BT Monocerotis The old nova BT Monocerotis

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..99...95s&link_type=abstract

(International Astronomical Union, Colloquium on Double Stars, Physical Properties and Generic Relations, 80th, Bandung, Indones

Astronomy and Astrophysics

Astrophysics

12

Eclipsing Binary Stars, Gas Streams, Novae, Stellar Models, H Alpha Line, Light Curve, Radial Velocity, Stellar Spectra, Stellar Winds

Scientific paper

Spectroscopic observations through most of the eclipse cycle of BT Mon reveal the presence of both low and high velocity gas streams. Acceleration through a Laval-nozzle-effect at the inner Lagrangian point of the system and powering of the emission lines through kinetic energy losses of Coriolis deflected and subsequently colliding gas streams are considered as possible mechanisms at work in the system.

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