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The termsgalactic corona andgaseous corona have been used in the first decade of the 21st century to describe a hot,ionised, gaseous component in thegalactic halo of theMilky Way. A similar body of very hot and tenuous gas in the halo of anyspiral galaxy may also be described by these terms.
The hypothetical source of the galactic halo ofcoronal gas may be the cumulative output of many “galactic fountains” in thegalactic disc ejecting hot gas.
The hypothesis is that a singlesupernova and then itssupernova remnant both produce hot ionized gas that supplies an individual “galactic fountain”. The expelled material forms agiant bubble of high-pressure, low density, hot gas in the denser, cooler gas and dust of thegalactic disc. At least some of those bubbles extend high or low enough, vertically, to pierce through the denser disk, and form “chimneys” which exhaust the hot gas into the halo, analogous to a terrestrialgeyser spewing out water and steam that is much hotter and much less dense than the surrounding earth, heated by a source hidden deep below.
As the expelled gas in the galactic corona cools, it falls back into thegalactic disc, guided by the disc's own gravitational attraction, enriching thegas and dust in the disc with the heavy elements (loosely termed“metals” by astronomers) which were produced in supernova precursors, and duringsupernova explosions.
Galactic coronas have been and are currently being studied extensively, in the hope of gaining a further understanding of galaxy formation.[1][2]However, considering how galaxies differ in shape and size, no particular theory has been able to adequately explain how all galactic coronas are formed and maintained.[3]
