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Theoretical Spectra
GRAMS, O-rich original grid (?)
Teff: - (?)
Logg: - (?)
Mass: - (?)
Rin: - (?)
τ10: - (?)

 
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Please, select the parameter values that you are interested in

Grids do not always have a uniform coverage of all the parameter space.
You can get a hint about grid coverage seeing what combinations of Tegg,Logg are available.


  
 

References:

  • GRAMS, O-rich original grid

    • 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
      Sargent et al 2011, ApJ 728, 93
 
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