Add the subsection on (finally!) calculating the dust density maximum. It's simply max(rho_d) = rho0*epsilon * (S+1), where rho0 is the maximum gas density, epsilon the global dust to gas ratio, and S=St/delta.
Merge branch 'master' of git://github.com/wlyra/transitional-disk

Conflicts:
	tex/trapping.tex
Added nonaxi to the Makefile.
updated figure 3 (include the effect of sedimentation)
minor changes: caption to fig 3, change in Sect 6 (observation prediction) with sedimentation; added total mass integration (should probablty merge the
end of Sect 4 into Sect 6).
minor text edits
Sending in my changes to merge with latest commit.
Merge branch 'master' of git://github.com/wlyra/transitional-disk
Highlight that the flow gets supersonic at some point, which limits the validity of the solution at large (x,y).
Finally done! Will do a last re-reading, and resubmit!
Removed red text (the referee may not have color printing).
Spell checked.
z -> zeta in Sect 5
Added section on dust contrast. :-)
Model sucessfully applied to Oph IRS 48!
updated the gas contrast, and the comparison with Oph IRS 48
Okay, that should be the end.

The paper has grown to 11 pages, which is not good. But I can't see what to cut.

The answer to the referee should follow soon. Hopefully the paper can be
resubmitted tonight.
Adding the report to the repository.
Added answer to the referee, plus a note of thanks to her in the aknowledgment
Added a header to the answer.