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| Paper: |
The Distribution of Warm Ionized Medium in Galaxies |
| Volume: |
438, The Dynamic Interstellar Medium: A Celebration of the Canadian Galactic Plane Survey |
| Page: |
179 |
| Authors: |
Haffner, L. M. |
| Abstract: |
Ionized nebulae have been targets of interest since the introduction of the telescope centuries ago.
These isolated, “classical” H II regions gave us some of the earliest insight into the
copious feedback energy that stars inject into the interstellar medium. Their unique spectra contain
information about the quality and quantity of the ionizing field as well as the temperature, density,
and metallicity of these discrete locations in the Galaxy. With increasing sensitivity across many
spectral domains, we now know that ionized gas is not localized to massive star regions in many
star-forming galaxies. In particular, recent observational studies allow a thorough comparison of
the physical conditions and distribution of the well-studied classical H II regions to the more
widespread warm, diffuse gas. By more realistically evolving a dynamic interstellar medium, models
are beginning to reproduce the observed emission measure variations and provide a natural solution
to the propagation of ionizing flux from a predominantly neutral galactic disk to the distant halo. |
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