The impact of high accuracy astrometry on asteroseismology

Articles in the same Issue

1. Contents
2. Proceedings of the Gaia Workshop
3. Gaia: the galactic central bulge
4. Predicting Gaia observations from a star-count model
5. Luminosity calibration and distance scale
6. The Cepheid-Based Distance Scale
7. The Spatial Resolution of the Extinction Structure from Gaia
8. The star formation history of the Milky Way: methodology and implications for Gaia
9. The velocity field and 3-D structure of the Universe
10. Prospects for astrometric measurements of gravitational waves from stellar sources with Gaia
11. Gaia and the evolution of young stars
12. Testing stellar structure and evolution with Gaia
13. Unraveling the history of star formation in the galactic disk with Gaia
14. A few remarks on AGB variable stars and the Gaia mission
15. Gaia science output: white dwarfs
16. On derivation of masses of the SB2 components with Gaia astrometry
17. The impact of high accuracy astrometry on asteroseismology
18. First thoughts about variable star analysis