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20002023
most citedLarge-Scale Structure of the Molecular Gas in Taurus Revealed by High Linear Dynamic Range Spectral Line Mapping

486 citations · 7.9k across the 158 of their papers we have counts for

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astro-ph2008★ 28 cited

Dichotomy in the Dynamical Status of Massive Cores in Orion

T. velusamy, R. Peng, D. Li +2

To study the evolution of high mass cores, we have searched for evidence of collapse motions in a large sample of starless cores in the Orion molecular cloud. We used the Caltech S…

astro-ph2008★ 41 cited

An Improved Technique for Measurement of Cold HI in Molecular Cloud Cores

Marko Krco, Paul F. Goldsmith, Robert L. Brown +1

The presence of atomic gas mixed with molecular species in a "molecular" cloud may significantly affect its chemistry, the excitation of some species, and can serve as probe of the…

astro-ph2008★ 49 cited

Resolving distance ambiguities towards 6.7 GHz methanol masers

J. D. Pandian, E. Momjian, P. F. Goldsmith

Distances to most star forming regions are determined using kinematics, through the assumption that the observed radial velocity arises from the motion of the source with respect t…

astro-ph2008★ 126 cited

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…

astro-ph2008★ 486 cited

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…