Towards asteroseismology of main-sequence g-mode pulsators: spectroscopic multi-site campaigns for slowly pulsating B stars and γ Doradus stars

Details Towards asteroseismology of main-sequence g-mode pulsators: spectroscopic multi-site campaigns for slowly pulsating B stars and γ Doradus stars Towards asteroseismology of main-sequence g-mode pulsators: spectroscopic multi-site campaigns for slowly pulsating B stars and γ Doradus stars

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1170..480d&link_type=abstract

STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION: Proceedings of the International Conference. AIP Conference Proceedin

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2

Pulsations, Oscillations, And Stellar Seismology, Gravitational Radiation, Magnetic Fields, And Other Observations, Photometric, Polarimetric, And Spectroscopic Instrumentation

Scientific paper

We introduce the spectroscopic multi-site campaigns that are organised
for a sample of slowly pulsating B and γ Doradus stars to make a
big step forward in the asteroseismic studies of these main-sequence
g-mode pulsators.

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