DIRTY Spherical Galacitic Environment Data

These tables were produced for the Clumpy Dust II paper. The tables were produced using dust grain properties derived from empirical work in the Milky Way and Small Magellanic Cloud.

Table 2	Table 3	Table 4
Dusty	Shell	Cloudy
ASCII	ASCII	ASCII

Full Original Data

Here are the all the runs computed for the Clumpy II paper. This data has more density ratios than presented in the Clumpy II paper.

The format of these files is different than those in Tables 2-4 of Clumpy II (above tables).

geometry, dust-type	k₂/k₁ (density ratio)
SHELL, MW	1.000 (homogeneous)	0.500	0.100	0.050	0.010 (clumpy)	0.005	0.001
SHELL, SMC	1.000 (homogeneous)	0.500	0.100	0.050	0.010 (clumpy)	0.005	0.001
DUSTY, MW	1.000 (homogeneous)	0.500	0.100	0.050	0.010 (clumpy)	0.005	0.001
DUSTY, SMC	1.000 (homogeneous)	0.500	0.100	0.050	0.010 (clumpy)	0.005	0.001
CLOUDY, MW	1.000 (homogeneous)	0.500	0.100	0.050	0.010 (clumpy)	0.005	0.001
CLOUDY, SMC	1.000 (homogeneous)	0.500	0.100	0.050	0.010 (clumpy)	0.005	0.001

2005 Update

This is the update to include a larger range of tau_V values and the addition of the LMC2 dust type.

The format of these files is the similar to the "Full Original Data" with more optical depths and more info at the top of the file.

geometry, dust-type	k₂/k₁ (density ratio)
SHELL, LMC2	1.000 (homogeneous)	0.010 (clumpy)
SHELL, SMC	1.000 (homogeneous)	0.010 (clumpy)
CLOUDY, LMC2	1.000 (homogeneous)	0.500	0.100	0.050	0.010 (clumpy)	0.005	0.001