Gaia Data Release 3. Pulsations in main sequence OBAF-type stars
Context. 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 M ⊙) of spectral types O, B
Gaia Collaboration et al.
Advertised on:
6
2023