Changes between Version 26 and Version 27 of u/erica/radtimescales


Ignore:
Timestamp:
04/04/16 15:04:50 (9 years ago)
Author:
Erica Kaminski
Comment:

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  • u/erica/radtimescales

    v26 v27  
    179179[[latex($\boxed{1 M_\odot =\rho l^3}$)]]
    180180
    181 Solving these equations equations gives:
     181This last equation is equivalent to setting the box radius = mean free path = scale height. Solving these equations equations gives:
    182182
    183183[[latex($h=l=.0068 ~pc$)]]
    184184
    185 ''' So a (uniform density) core that contains a solar mass, has to be .0068 to be optically thick. That is an interesting result. '''
     185''' So a (uniform density) core that contains a solar mass, has to be .0068 ~pc to be nearly optically thick. That is an interesting result. '''
    186186
    187187Recalculating the sims parameters, and diffusion time, gives: