Numerical simulations of convection in A-stars

Details Numerical simulations of convection in A-stars Numerical simulations of convection in A-stars

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..224..139f&link_type=abstract

The A-Star Puzzle, held in Poprad, Slovakia, July 8-13, 2004. Edited by J. Zverko, J. Ziznovsky, S.J. Adelman, and W.W. Weiss,

Other

11

Convection, Hydrodynamics, Radiative Transfer, Methods: Numerical, Stars: Atmospheres.

Scientific paper

Radiation hydrodynamics simulations have been used to produce numerical
models of the convective surface layers of a number of stars, including
the Sun and other stars on or above the main-sequence, white dwarfs of
type DA, and red supergiants.

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