Velocity field in the fragmented molecular cloud core of W3 - Evidence for large-scale turbulence

Details Velocity field in the fragmented molecular cloud core of W3 - Evidence for large-scale turbulence Velocity field in the fragmented molecular cloud core of W3 - Evidence for large-scale turbulence

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...340..298h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 340, May 1, 1989, p. 298-306.

Astronomy and Astrophysics

Astrophysics

40

Interstellar Chemistry, Molecular Clouds, Molecular Rotation, Turbulence, Carbon Monoxide, Gravitational Effects, H Ii Regions

Scientific paper

High-resolution observations of the core region of the W3 molecular cloud using the (C-13)O emission as well as HCO+ and HCN emissions are reported. A high-resolution map of the optically thin (C-13)O emission is presented which is free from the self-reversal at V(LSR) = -39 km/s and which clearly reveals the detailed structure and the velocity field of W3 core. The complicated velocity field seen in the core is resolved into the relative and internal motions of the two condensations.

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