CaII and NaI absorption signatures from the circumgalactic gas of the Milky Way
arXiv:0708.1855 · doi:10.1007/978-1-4020-6933-8_61
Abstract
We combine CaII/NaI absorption and HI 21 cm emission line measurements to analyse the metal abundances, the distribution, the small-scale structure, and the physical conditions of intermediate- and high-velocity gas in the Galactic halo.
2 pages, 1 figure, to appear in proceeding of "Galaxies in the Local Volume" Sydney 8-13 July 2007
References in corpus (3)
- The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections
- New perspectives on strong z=0.5 MgII absorbers: are halo-mass and equivalent width anti-correlated?
- Low-column density gas clumps in the halo of the Milky Way