Galactic corona
From Wikipedia, the free encyclopedia
The term galactic corona has been used in the first decade of the twenty-first century to describe a hot, ionised, gaseous component of the Milky Way.
[edit] See also
- Galaxy formation and evolution
- Galactic coordinate system
- Galactic bulge
- Disc galaxy
- Galactic halo
- Galactic spheroid
[edit] External links
- THE GALACTIC CORONA, Jerry Bonnell, 1995
- Absorption Line Studies in the Halo, Philipp Richter, 2003
- Multi-phase High-Velocity Clouds toward HE 0226-4110 and PG 0953+414, Andrew J. Fox et.al., 2005
- Galactic Corona or Local Group Intergalactic Medium?, Rik J. Williams, Smita Mathur, & Fabrizio Nicastro, 2005
- NGC 5746: Detection of Hot Halo Gets Theory Out of Hot Water