Diffuse ionized gas in nearby GalaxiesWe discuss the distribution and spectral characteristics of diffuse ionized gas in nearby galaxies. The diffuse gas has been mapped in both edge-on and more face-on galaxies providing information on the radial and vertical distributions. Emission from diffuse ionized gas is strongest around star forming regions. The vertical distribution appears related to the radio continuum thick-disk emission. We also briefly discuss ionization mechanisms and the connection between star formation characteristics and morphology of the interstellar medium.
Document ID
19930035023
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Walterbos, R. A. M. (California Univ. Berkeley, United States)
Date Acquired
August 15, 2013
Publication Date
January 1, 1991
Publication Information
Publication: In: The interstellar disk-halo connection in galaxies (A93-18998 05-90)