A grid of MARCS model atmospheres for late-type stars I. Methods and general properties
Uppsala University · Astronomy and Space · +2 more institutions
Abstract
We have constructed a grid of about 10,000 spherically symmetric and plane-parallel models with the MARCS program, and make it available for public use. Parameter ranges are: Teff=2500 to 8000 K, log g =log(GM/R2)= -1 to 5 (cgs) with various masses and radii, [Me/H]=-5 to +1, with [Alpha/Fe] = 0.0 and 0.4 and different choices of C and N abundances to also represent stars of types R, S and N, and with microturbulence parameters from 1 to 5 km/s. We also list fluxes in approximately 108,000 wavelength points. Underlying assumptions in addition to 1D stratification include hydrostatic equilibrium, MLT convection and LTE. A number of general properties of the models are discussed, in relation to the effects of…
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Authors
6- BGB. GustafssonCorresponding
Uppsala University, Astronomy and Space
- BEB. Edvardsson
Uppsala University, Astronomy and Space
- EKEriksson, Kjell
Uppsala University, Astronomy and Space
- UGU. G. Jørgensen
University of Copenhagen
- ÅNÅke Nordlund
University of Copenhagen
Topics & keywords
- Physics
- Astrophysics
- Stars
- Blanketing
- Hydrostatic equilibrium
- Spectral line
- Stellar atmosphere
- Opacity