Galactic Winds and the Hubble Sequence |
Common terms and phrases
ablation accumulation addition assumed become Bergh bulge cluster component conduction constant continued Cowie crit decreases density dependent depleted detailed determine develop discussed disk early galactic winds effect elliptical energy equations escape exist exterior Faber and Gallagher field Figure flow Freeman frequency function galactic gas galaxy Gallagher 1976 gas depletion gas-poor greater halo heating important increases initial interior halo internal less lines mass loss rate massive Mathews mean models nature necessary numerical observations occurs outer parameter partial wind passes photographed potential pressure probably radiation radiative cooling radio radius range ratio region remain result rotational Sandage scale shock specific spherical spirals star formation stars steady stellar stripped suggest supernova supernova heating surface temperature thermalized total winds University values velocity dispersion Virgo X-ray core