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Changes between Version 18 and Version 19 of u/NewUsers

v18	v19
31	31	Now, sometimes insufficient resolution can impede the formation of sinks. If you have a zone that has exceeded the density threshold, you may work through some algebra to show the size of dx that is required for collapse. Also, there are a series of print statements in the subroutine mentioned above that you can uncomment. This will show you what has passed and what has not.
32	32
33		The sink routines are more or less taken from [http://adsabs.harvard.edu/abs/2010ApJ...713..269F Federrath et al]. I have added a summary of this paper and its findings on my page, under the library section.
	33	The sink routines are more or less taken from [http://adsabs.harvard.edu/abs/2010ApJ...713..269F Federrath et al]. I have added a summary of this paper and its findings on my page, under the library section. Also, note that the accretion radius is 4dx: IR_ACC = 4, as defined in particle_declarations.f90 and is used in particle_control.f90 to set r_acc.
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35	35	== Effectively Implementing AMR ==