VizieR Online Data Catalog: M-type AGB stars wind and dust models (Bladh+, 2019)

We present an extensive grid of dynamical atmosphere and wind models for M-type AGB stars, covering a wide range of relevant stellar parameters. We used the DARWIN code, which includes frequency-dependent radiation- hydrodynamics and a time-dependent description of dust condensation and evaporation, to simulate the dynamical atmosphere. The wind-driving mechanism is photon scattering on submicron-sized Mg₂SiO₄ grains. The models produce radial snapshots of the atmospheric structure, dynamical properties (mass-loss rates and wind velocities) and dust properties (grain sizes, dust-to-gas ratios, and degree of condensed Si).

Fundamental model parameters (stellar, dust, and pulsation parameters) and the resulting wind and dust characteristics for DARWIN models of M-type AGB stars producing a stellar wind.

(1 data file).