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The Five College Radio Astronomy Observatory CO Mapping Survey of the Taurus Molecular Cloud
Gopal Narayanan, Mark H. Heyer, Christopher Brunt +3
The FCRAO Survey of the Taurus Molecular Cloud observed the 12CO and 13CO J=1-0 emission from 98 square degrees of this important, nearby star forming region. This set of data with…
Large-Scale Structure of the Molecular Gas in Taurus Revealed by High Linear Dynamic Range Spectral Line Mapping
Paul F. Goldsmith, Mark Heyer, Gopal Narayanan +3
We report the results of a 100 square degree survey of the Taurus Molecular Cloud region in the J = 1-0 transition of 12CO and 13CO. The image of the cloud in each velocity channel…
The Transition from Atomic to Molecular Hydrogen in Interstellar Clouds: 21cm Signature of the Evolution of Cold Atomic Hydrogen in Dense Clouds
Paul F. Goldsmith, Di Li, Marko Krco
We have investigated the time scale for formation of molecular clouds by examining the conversion of HI to H2 using a time-dependent model. H2 formation on dust grains and cosmic r…
The COMPLETE Survey of Star-Forming Regions: Phase I Data
Naomi A. Ridge, James Di Francesco, Helen Kirk +14
We present an overview of data available for the Ophiuchus and Perseus molecular clouds from ``Phase I'' of the COMPLETE Survey of Star-Forming Regions. This survey provides a rang…
HI Narrow Self-Absorption in Dark Clouds: Correlations with Molecular Gas and Implications for Cloud Evolution and Star Formation
P. F. Goldsmith, D. Li
We present the results of a comparative study of HI narrow self-absorption (HINSA), OH, 13CO, and C18O in five dark clouds. The HINSA follows the distribution of the emission of th…
Observations of Water Vapor Outflow from NML Cygnus
Viktor Zubko, Di Li, Tanya Lim +2
We report new observations of the far infrared and submillimeter water vapor emission of NML Cygnus based on data gathered with the Infrared Space Observatory and the Submillimeter…