β1 Monocerotis: oscillations and chromospheric structure

Details β1 Monocerotis: oscillations and chromospheric structure β1 Monocerotis: oscillations and chromospheric structure

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...286..160m&link_type=abstract

Astronomy and Astrophysics 286, 160-168 (1994)

Astronomy and Astrophysics

Astrophysics

2

Stars: Emission-Line, Be, Stars: Chromospheres, Stars: Oscillations, Stars: Mass-Loss

Scientific paper

β1 Monocerotis is a Be star with a V/R cycle of 12.5 years. We
observed the star from CTIO (Chile) and with the IUE satellite and found
that the star undergoes photospheric oscillations of 1.7 hours and
presents a chromospheric structure in the extended atmosphere. Infall
velocities and ejection of material are discussed.

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