Synthetic Photometry
Model:
Bayo et al, M types from Collinder 69
Complete M spectral type sequence for a sample of confirm young sources (members of Collinder 69, ~5-20 Myr). Be aware that most spectra are not flux calibrated.
Model parameters
SpTy:(?)

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λmean:- A
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References:

  • Bayo et al 2011, A&A 536, 63B
    Spectroscopy of very low mass stars and brown dwarfs in the Lambda Orionis star forming region. I. Enlarging the census down to the planetary mass domain in Collinder 69
     
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