Computer Science
Scientific paper
Feb 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978natur.271..730d&link_type=abstract
Nature, vol. 271, Feb. 23, 1978, p. 730, 731.
Computer Science
6
Hydrogen Ions, Interstellar Radiation, Lyman Alpha Radiation, Photoionization, H Ii Regions, Interstellar Gas, Luminous Intensity, Supernovae
Scientific paper
Consideration of photoionized H II regions, shock-heated gas, and collisional excitation and recombination in interstellar H I leads to the conclusion that the mean Lyman-alpha intensity in interstellar H I is at most three times 10 to the minus fifth power erg per sq cm per sec per steradian. This finding would tend to undermine assertions that Lyman-alpha may play an important part in photoemission from interstellar grains. Moreover, Lyman-alpha intensity surrounding supernovae and H II regions is frequently found to be very large compared to the continuum background in the 10.2-13.6 eV band.
Draine Bruce T.
Salpeter Edwin E.
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