Non-radial pulsations in Be stars

Details Non-radial pulsations in Be stars Non-radial pulsations in Be stars

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.538..289b&link_type=abstract

In: Second Eddington Workshop: Stellar structure and habitable planet finding, 9 - 11 April 2003, Palermo, Italy. Edited by F. F

Physics

Stars: Emission-Line, Be Stars: Oscillations

Scientific paper

Be stars (i.e. stars with emission lines) represent nearly 20% of B stars. Non-radial pulsations in Be stars were discovered more than twenty years ago and asteroseismology is the only way to study the internal structure of these stars. It may also provide clues to understand the so far unexplained formation of their circumstellar envelopes in which emission originates. A review of results obtained is presented, as well as future progress expected from Eddington observations.

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