The Astrophysical Journal · 1998 · 168 citations · 35 references
Natural SciencesAstronomyPhysicsAtmospheric ScienceInterstellar MediumMolecular PhysicsInterstellar GasInterstellar TurbulenceMolecular CloudsTurbulenceTurbulent FlowTurbulent MixingDense Molecular CoresDense Molecular GasH I TurbulenceLine WidthTurbulence In Molecular CloudsVelocity Dispersion Profiles
In a study of the velocity dispersion of molecular gas in maps of four dense cores, we nd that : NH 3 (1) within the interiors of dense cores, the line widths are roughly constant at a value slightly but signicantly higher than a purely thermal line width ; and (2) at the edges of the maps of the dense cores, it appears that the line width starts to increase. We suggest that these dense cores are "" coherent in that the nonthermal, turbulent, contributions to the line width are so small that observed velocity dispersion is nearly independent of scale within the cores. In the second paper of this series (Goodman et al.), by analyzing maps of the cores environments, we nd an apparent transition to this coherent regime from a more turbulent one, at about the size scale of a FWHM contour, or D0.1 pc. NH 3 Analysis of velocity gradients in dense cores and their environs indicates that the cores appear to spin independently of their surroundings, along an axis not obviously related to their shape. Comparison of gradients implied by the relative velocities of high-density cores in complexes and gradients in the extended low-density gas in these complexes suggests a picture in which the coherent cores behave as (independently spinning) test particles, oating along in a turbulent ow.
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Mass, luminosity, and line width relations of Galactic molecular clouds
P. M. Solomon, A. R. Rivolo, John W. Barrett et al. · The Astrophysical Journal · 1987 · 1.6K citations
Natural Sciences, Astronomy, Physics +13
Dense cores in dark clouds. VIII - Velocity gradients
Alyssa Goodman, P. J. Benson, G. A. Fuller et al. · The Astrophysical Journal · 1993 · 697 citations
Natural Sciences, Astronomy, Physics +12