… approximate results of Castor, McCray, and Weaver. The effect of stellar motion on the
structure … The appropriate subsonic solution is determined by the values above for v, p�…

… of Castor, McCray, and Weaver. The effect of stellar motion on the structure of a bubble, the
hydrodynamic stability of the outer shell, and the observable properties of the hot region and …

… authors had failed to adopt the center-of-mass coordinates for the colliding pair in the calculation
of Q(r). The … r 1 3T 3~2 3 3J~2 Q(p) ~ ~ + 2p”2 — — a0 + (_) a1p — ~ (_) a1p512], (18) …

… origins in material swept up by stellar winds (Castor, McCray & Weaver 1975, Weaver et
al. 1977). The detailed … dense downstream flow may break up into sheets or filaments (McCray, …

Correlated supernovae from an OB association create a superbubble: a large, thin, shell of
cold gas surrounding a hot pressurized interior. Because supernova blast waves usually�…

… where the density at the galactic plane is p~ = 2.1 1 x 10 24 g … (1) having log p = -26.977 to
the highest (10) having log p = -… derived following the spherical bubble solution of Weaver et …