The warm ionized medium in spiral galaxies

Bibcode
2009RvMP...81..969H
DOI
10.1103/RevModPhys.81.969
Haffner, L. M.; Dettmar, R.-J.; Beckman, J. E.; Wood, K.; Slavin, J. D.; Giammanco, C.; Madsen, G. J.; Zurita, A.; Reynolds, R. J.
Bibliographical reference

Reviews of Modern Physics, vol. 81, Issue 3, pp. 969-997

Advertised on:
7
2009
Journal
Reviews of Modern Physics
Number of authors
9
IAC number of authors
2
Citations
319
Refereed citations
290
Description
This article reviews observations and models of the diffuse ionized gas that permeates the disk and halo of our Galaxy and others. It was inspired by a series of invited talks presented during an afternoon scientific session of the 65th birthday celebration for Professor Carl Heiles held at Arecibo Observatory in August 2004. This review is in recognition of Carl’s long-standing interest in and advocacy for studies of the ionized as well as the neutral components of the interstellar medium.
Related projects
Poster Almeria Astronomy week
Kinematic, Structural and Composition Studies of the Interstellar and Intergalactic Media
The basic objective of the broject is to investigate the evolution of galaxies by deepening our understanding of the interaction between the insterstellar medium and the stars.The main technique which we use is the two-dimensional kinematic study of whole galaxies observed using our instrument:GHaFaS, a Fabry-Perot interferometer on the William
Prof.
John E. Beckman
In progress
Type
Refereed
Formation & Evolution of Galaxies (FYEG)

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