In this paper the authors have presented the preliminary results of observations undertaken to study the physics and chemistry of the dark cloud L134N. The observations indicate that the dark cloud L134N has a complex physical and chemical constitution. Rotational emission lines from the carbon monoxide isotope, 13CO, indicate the large scale structure and kinematics of the cloud, but fail to indicate the high density core.
Masers, Molecules, and Mass Outflows in Star Formation Regions
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