Microwave H2O emission from young stars

Details Microwave H2O emission from young stars Microwave H2O emission from young stars

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...201l..27s&link_type=abstract

Astrophysical Journal, vol. 201, Oct. 1, 1975, pt. 2, p. L27, L28.

Astronomy and Astrophysics

Astrophysics

41

A Stars, B Stars, Early Stars, Interstellar Gas, Stellar Evolution, Microwave Radiometers, Microwave Spectra, Radiation Sources, Stellar Radiation, T Tauri Stars

Scientific paper

H2O emission has been detected from the Ae or Be stars HD 250550, LkH-alpha 234, and LkH-alpha 198. Comparison of the H2O velocity with that of associated interstellar CO indicates that the H2O originates in an infall region, possibly the contracting parent cloud. H2O emission has also been detected in OH 205.1-14.1, and OH source near the T Tauri star LkH-alpha 308.

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