Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...228..197n&link_type=abstract
Astrophysical Journal, Part 1, vol. 228, Feb. 15, 1979, p. 197-205. Research supported by the University of California
Astronomy and Astrophysics
Astronomy
195
Herbig-Haro Objects, Hydrogen Clouds, Interstellar Matter, Main Sequence Stars, Stellar Evolution, Stellar Models, Water Masers, Cloud Physics, Collisional Plasmas, Cosmic Dust, Gas Dynamics, Infrared Astronomy, Magnetohydrodynamic Stability, Stellar Mass Ejection, Stellar Winds, Supersonic Flow
Scientific paper
The paper considers the energy input to H2O masers in a dense molecular cloud and analyzes the response time scales for both collisional and radiative pump models. Specific mechanisms for magnetic energy input are given. The evolution of dense H2O maser clouds is studied in the environment of a young pre-main-sequence star that has developed an appreciable supersonic wind. It is shown that compact clouds can be ejected at high velocity to distances of order 1 pc. It is suggested that these clouds (referred to as interstellar bullets) might explain the phenomena of Herbig-Haro objects and high-velocity gas motions observed near compact infrared objects.
Norman Colin
Silk Joseph
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