NASA NTRS · 19720030859
Radiofrequency recombination lines as diagnostics of the cool interstellar medium.
Abstract
Quantitative details are given of a new diagnostic technique for the carbon and hydrogen (H I) recombination lines. Theoretical results are presented for conditions expected in H I clouds, and are compared with available observations for Orion A and NGC 2024.
Keep this discovery
Explore connections, maps & timelines
Dupree, A. K.. 1971-12-15. Radiofrequency recombination lines as diagnostics of the cool interstellar medium.. https://ntrs.nasa.gov/citations/19720030859
Cite the original work for its findings. Save a collection to share your selection of sources.