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Gaia Data Release 3: Pulsations in main sequence OBAF-type stars

By Gaia Collaboration and others
The third Gaia data release provides photometric time series covering 34 months for about 10 million stars. For many of those stars, a characterisation in Fourier space and their variability classification are also provided. This paper focuses on intermediate- to high-mass (IHM) main sequence pulsators M >= 1.3 Msun) of... Show more
August 16, 2022
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Gaia Data Release 3: Pulsations in main sequence OBAF-type stars
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