Titlebook: Radio Recombination Lines: 25 Years of Investigation; Proceeding of the 12 M. A. Gordon,R. L. Sorochenko Conference proceedings 1990 Kluwer

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R. L. Sorochenko,G. T. Smirnovle accuracy and data utility must remain high. Our methodology aims at protecting audio files and users’ identities through the use of encryption and hashing algorithms, while at the same time providing accurate speaker’s identity prediction. In addition, for speech recognition, we introduce a mecha

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Radio Recombination Lines from Compact HII Regions The line to continuum ratios are spread over a much wider range than that span by extended regions. We show that the large ratios are due to line enhancement by stimulated emission, while the small ones can be attributed to line suppression in regions with large continuum opacities.

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Radio Recombination Lines at Millimeter Wavelengths in HII Regionsd by Salem and Brocklehurst (1979)..This review is intended to cover the salient features of radio recombination lines (RRLs) at millimeter wavelengths but excludes discussion of the mm-wave maser lines from the star MWC349, which is described in a separate article in this volume.

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Radio Recombination Lines from Stellar Envelopes: Planetary Nebulaed although we have made significant progress, we do not yet have a satisfactory detailed understanding of the entire evolutionary progression of the formation of planetary nebulae (see for example the most recent IAU Symposium Proceedings; ., 1989, ed. S. Torres-Peimbert).

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