Interpretation of type I OH maser sources

Details Interpretation of type I OH maser sources Interpretation of type I OH maser sources

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980natur.286..136k&link_type=abstract

Nature, vol. 286, July 10, 1980, p. 136-138. Deutsche Forschungsgemeinschaft

Computer Science

4

Hydroxyl Radicals, Interstellar Masers, Electron Transitions, Hyperfine Structure, Infrared Radiation, Molecular Spectra, Pumping

Scientific paper

OH maser sources of type I, which are related to regions of star formation, have been known for more than a decade. However, despite great effort no satisfactory theoretical interpretation has yet been given. A model for the interpretation of type I OH maser sources is suggested here. This model combines the effect of velocity and magnetic field gradients with radiative pumping by means of the (2 Pi 3/2, J equals 5/2 to 2 Pi 1/2, J equals 5/2) transition. Due to an overlap of particular hyperfine components, inversion of the 1665 MHz line is favored.

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