Discovery of Hydroxyl Radio Emission from Infrared Stars

Details Discovery of Hydroxyl Radio Emission from Infrared Stars Discovery of Hydroxyl Radio Emission from Infrared Stars

Aug 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968sci...161..778w&link_type=abstract

Science, Volume 161, Issue 3843, pp. 778-779

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94

Scientific paper

Radio spectral line emission from hydroxyl radicals has been detected
from four infrared stars. The emission from the infrared star NML Cygni
at 1612 megahertz is the strongest radio emission line yet detected.
Sixteen other stars with infrared excesses showed no detectable hydroxyl
radio emission.

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