The Size Distribution of Superbubbles in the Interstellar Medium
M.S. Oey & C.J. Clarke
(This is a user-friendly summary of Oey & Clarke
1997 , plus N(v) derivation.)
We use the standard, adiabatic shell evolution to predict the
size distribution N(R) for populations of SN-driven superbubbles
in a uniform
ISM. We derive N(R) for simple cases of superbubble creation rate and
mechanical luminosity function. We then compare our predictions
for N(R) with the largely complete H I hole catalogue for the SMC,
with a view toward the global structure of the ISM in that galaxy. We
also present a preliminary derivation for N(v), the distribution of
shell expansion velocities.
1998, in "Interstellar Turbulence," eds. J. Franco &
A. Carraminana, Cambridge U. Press, in press
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