Changes between Version 9 and Version 10 of u/erica/RadFeedback


Ignore:
Timestamp:
11/19/15 12:13:59 (9 years ago)
Author:
Erica Kaminski
Comment:

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  • u/erica/RadFeedback

    v9 v10  
    1111[[latex($\frac{1}{2} m v_{ff}^2 = \frac{GmM}{r}$)]]
    1212
    13 As the material strikes the surface of the star (i.e. is accreted) the kinetic energy is then converted to heat. For an accretion rate [[latex($\dot{m}$)]], the rate at which this heat is released, or the luminosity L, is given by:
     13As the material strikes the surface of the star (i.e. is accreted) the kinetic energy is converted to heat. For an accretion rate [[latex($\dot{m}$)]], the rate at which this heat is released, or the luminosity L, is given by:
    1414
    1515[[latex($ L = \frac{1}{2}\dot{m} v_{ff}^2 = \dot{m}\frac{GM}{r}$)]]