Results from Classification Observations and a Multi-site Campaign on γ Doradus and SPB Type Stars

Details Results from Classification Observations and a Multi-site Campaign on γ Doradus and SPB Type Stars Results from Classification Observations and a Multi-site Campaign on γ Doradus and SPB Type Stars

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1170..467w&link_type=abstract

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

Computer Science

1

Low-Amplitude Blue Variables, Pulsations, Oscillations, And Stellar Seismology, Main-Sequence: Early-Type Stars

Scientific paper

As part of a observational project aiming to investigate the effects of rotation on main-sequence g-mode non-radial pulsation we have obtained at least one (generally more) high-resolution spectroscopic observation of more than 50 confirmed or candidate γ Doradus and slowly pulsating B stars and have completed a spectroscopic multi-site campaign. The campaign was one of those outlined in De Cat et al. (these proceedings) and included five observatories and focused on the γ Doradus, and now planet hosting star HD 218396 (HR 8799) and the SPB stars HD 21071 and HD 25558.

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