Pulsating B Stars observed by Kepler

Details Pulsating B Stars observed by Kepler Pulsating B Stars observed by Kepler

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21934804m&link_type=abstract

American Astronomical Society, AAS Meeting #219, #348.04

Astronomy and Astrophysics

Astronomy

Scientific paper

In a prior investigation using Kepler data, Balona et al. (2011) found that the measured frequency spectra of B stars differed from those obtained using ground-based observations. The low amplitude frequency spectra of these stars are quantified by analyzing a larger number of B stars. These stars are then categorized using the designations adopted in the Balona et al. study. Most of the frequencies we measure are too small to be detected using conventional ground-based observations. They are probably associated with higher order spherical harmonic modes. A plan to determine the l values of the larger amplitude B star frequencies is presented.

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