Synthetic Photometry
Model:
GRAMS, O-rich original grid
GRAMS (Grid of Red supergiant and Asymptotic giant ModelS) is a grid of radiative transfer (RT) models for dust shells around red supergiant (RSG) and asymptotic giant branch (AGB) stars. This is the model grid for Oxygen-rich stars
Model parameters
Teff: - (?)
Logg: - (?)
Mass: - (?)
Rin: - (?)
τ10: - (?)

Show:

Filters
Show only filters with:
λmean:- A
Facility
Instrument
(You can select 50 filters at most, the rest will be ignored)
Please, select the parameter values that you are interested in
 

References:

  • GRAMS website
  • Sargent et al 2011, ApJ 728, 93
    The Mass-loss Return from Evolved Stars to the Large Magellanic Cloud. IV. Construction and Validation of a Grid of Models for Oxygen-rich AGB Stars, Red Supergiants, and Extreme AGB Stars
     
© CAB 2008