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Neutral Gas Contributions to [S II] Galactic Background Emission
Published online by Cambridge University Press: 25 May 2016
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Elevated ratios of [S II]/Hα relative to those typical of H II regions have been used to identify supernova remnants (SNRs) and also characterize the diffuse Galactic background (Reynolds 1985) and gas observed on the large scale in other galaxies (e.g., Lehnert & Heckman 1994). We explore the implications for these regions of the fact that ionized sulfur may exist both in gas that is predominantly neutral as well as fully ionized.
- Type
- Chapter 7: How are we to Understand the Small Scale Structure of the ISM?
- Information
- Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 613 - 614
- Copyright
- Copyright © Kluwer 1996
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