Changes between Version 24 and Version 25 of u/erica/scratch4

Timestamp:

02/16/16 19:56:41 (9 years ago)

Author:

Erica Kaminski

Comment:

—

u/erica/scratch4

@@ -23 +23 @@
 At each time step i, the luminosity is computed as:
 
-[[latex($L_i=\frac{G M_i dm_i}{R ~dt}$)]]
+[[latex($L_i=\frac{G M_i dm_i}{R }$)]]
 
 where [[latex($M_i$)]] is the mass of the sink particle at time i, [[latex($dm_i$)]] is the total accreted mass for that time step, [[latex($G$)]] is the gravitational constant in computational units, [[latex($R$)]] is the radius of the star, taken to be 1 solar radius by default, but modifiable by the user at run-time.