Galactic corona
 | This article includes a list of references, related reading, or external links, but its sources remain unclear because it lacks inline citations. (December 2020) |
|
The terms galactic corona and gaseous corona have been used in the first decade of the 21st century to describe a hot, ionised, gaseous component in the galactic halo of the Milky Way. A similar body of very hot and tenuous gas in the halo of any spiral galaxy may also be described by these terms.
Current hypothetical scenario
[edit]The hypothetical source of the galactic halo of coronal gas may be the cumulative output of many “galactic fountains” in the galactic disc ejecting hot gas.
The hypothesis is that a single supernova and then its supernova remnant both produce hot ionized gas that supplies an individual “galactic fountain”. The expelled material forms a giant bubble of high-pressure, low density, hot gas in the denser, cooler gas and dust of the galactic 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 terrestrial geyser 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 the galactic disc, guided by the disc's own gravitational attraction, enriching the gas and dust in the disc with the heavy elements (loosely termed “metals” by astronomers) which were produced in supernova precursors, and during supernova explosions.
Current research
[edit]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]
See also
[edit]- Galaxy formation and evolution
- Galactic coordinate system – Celestial coordinate system in spherical coordinates, with the Sun as its center
- Galactic bulge – Tightly packed group of stars within a larger formation
- Disc galaxy – Type of galactic form
- Spiral arm – Spiral-shaped regions of enhanced brightness within the galactic disc in spiral galaxies
- Galactic halo – Spherical component of a galaxy which extends beyond the main, visible component
- Galactic spheroid – Class of galaxy that has spiral structures extending from their cores.
References
[edit]- ^ Pedersen, K.; et al. (X-ray: NASA / CXC / U. Copenhagen; optical: Palomar DSS) (2006). Detection of hot halo gets theory out of hot water. Chandra Space Telescope (composite optical & X-ray image with expository caption). NGC 5746. Harvard University. Retrieved 19 December 2020.
- ^ Williams, Rik J.; Mathur, Smita & Nicastro, Fabrizio (2005). "Galactic corona or Local Group intergalactic medium?". arXiv:astro-ph/0511621.
- ^ Hille, Karl (22 September 2017). "Hubble's cool galaxy with a hot corona". NASA.gov. Retrieved 25 September 2017.
External links
[edit]- Bonnell, Jerry (1995). "The galactic corona".
- Richter, Philipp (2003). "Absorption line studies in the halo". How does the Galaxy Work?. Astrophysics and Space Science Library. Vol. 315. pp. 129–135. arXiv:astro-ph/0309693. doi:10.1007/1-4020-2620-X_22. ISBN 1-4020-2619-6. S2CID 14742733.
- Fox, Andrew J.; et al. (2005). "Multi-phase high-velocity clouds toward HE 0226-4110 and PG 0953 414". Astrophys. J. 630 (1): 332–354. arXiv:astro-ph/0505299. Bibcode:2005ApJ...630..332F. doi:10.1086/431915. S2CID 2545271.
