ar X iv : a st ro - p h / 98 03 06 9 v 1 6 M ar 1 99 8 The Size Distribution of Superbubbles in the Interstellar Medium
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چکیده
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.
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تاریخ انتشار 1998