3D hydrodynamical simulations of stellar surfaces : Applications to Gaia

Details 3D hydrodynamical simulations of stellar surfaces : Applications to Gaia 3D hydrodynamical simulations of stellar surfaces : Applications to Gaia

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sf2a.conf....3b&link_type=abstract

"SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: C. Charbonnel, F. Combes

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

We use 3D time-dependent hydrodynamical simulations to model the
photospheres of late type stars in a very realistic way. We apply these
simulations to study the 3D line formation in the spectral domain of the
spectrometer on board in the space mission Gaia.

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