POLYTROPIC STAR SKETCH - M,R type or M,L,T type. Use properties of Main Sequence stars (V) for input. Spec Teff M/Msun R/Rsun L/Lsun ro_avg (After O5 40000 39.811 17.783 501187 0.01 Bowers & B0 28000 17.783 7.413 19953 0.063 Deeming) B5 15500 6.457 3.802 794.33 0.166 Note that A0 9900 3.236 2.512 79.43 0.282 collapsors A5 8500 2.089 1.738 19.95 0.5495 with F0 7400 1.698 1.349 6.31 0.9772 Lnuc << L F5 6580 1.288 1.202 2.512 1.0715 may be modeled G0 6030 1.0965 1.0417 1.259 1.3489 with n=1.5 G5 5520 0.9333 0.9333 0.794 1.5849 or n=3. Then K0 4900 0.7762 0.8514 0.398 1.7783 L = K5 4130 0.6918 0.7413 0.1585 2.3988 A*MAX(L_radiative), M0 3480 0.4977 0.631 0.0631 2.5119 1 < A < 2, M5 2800 0.2138 0.3162 0.00794 10.0 where the upper M8 2400 0.1 0.1259 0.000794 63.1 limit is speculative. INPUTS: Mass in solar masses, Polytropic_type: n=3 or n=1.5, Radius in solar radii, the observed Luminosity in solar units, Stellar Chemistry, Model_Star_Name, Model_Distance in LY. $