High-density gas associated with 'molecular jets' - NGC 1333 and NGC 2071

Details High-density gas associated with 'molecular jets' - NGC 1333 and NGC 2071 High-density gas associated with 'molecular jets' - NGC 1333 and NGC 2071

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...267l.109s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 267, April 15, 1983, p. L109-L114.

Astronomy and Astrophysics

Astrophysics

48

Carbon Monoxide, Early Stars, Interstellar Gas, Interstellar Radiation, Stellar Winds, Ammonia, Gas Density, Molecular Clouds

Scientific paper

The high-density gas associated with broad-winged bipolar CO emission in NGC 1333 and NGC 2071 have been observed by mapping objects in C-18O, NH3 (1,1), and CS (J = 3-2). The general structure of high-density interstellar gas near these objects is elongated orthogonal to the separation of the red and blue high-velocity CO components. This suggests that a stellar wind is interacting with a primarily planar parent cloud, snowplowing material into a lumpy, high-density torus in the plane of the cloud and excavating a cavity containing high-velocity, low-density gas perpendicular to the plane of the cloud.

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