| Literature DB >> 16592999 |
Abstract
Spectral line intensity data are presented for ionized hydrogen regions in the giant spiral galaxy M101. The influence of interstellar extinction is assessed and electron temperatures of the gas clouds are derived.Entities:
Year: 1981 PMID: 16592999 PMCID: PMC319268 DOI: 10.1073/pnas.78.4.1994
Source DB: PubMed Journal: Proc Natl Acad Sci U S A ISSN: 0027-8424 Impact factor: 11.205