H2O masers near OB associations

Details H2O masers near OB associations H2O masers near OB associations

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...227..152b&link_type=abstract

Astrophysical Journal, Part 1, vol. 227, Jan. 1, 1979, p. 152-158.

Other

70

Interstellar Masers, Protostars, Star Clusters, Water Masers, Astronomical Spectroscopy, B Stars, Carbon Monoxide, Hydrogen Clouds, Interstellar Matter, O Stars, Radial Velocity, Stellar Evolution

Scientific paper

Four new water masers have been found in the vicinity of three OB associations. One of these, in Cep OB3, is among the most intense sources yet discovered and may be related to the most recent epoch of star formation in the OB association. Two others, one in CMa OB1, the other in M16, have large radial velocities relative to their associated molecular clouds. These results are discussed in the context of star formation and CO line self-reversal within the individual sources.

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