A molecular line study of a bipolar outflow object NGC 2071-north in L1630

Details A molecular line study of a bipolar outflow object NGC 2071-north in L1630 A molecular line study of a bipolar outflow object NGC 2071-north in L1630

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...325..372i&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 325, Feb. 1, 1988, p. 372-381.

Astronomy and Astrophysics

Astrophysics

26

Molecular Clouds, Nebulae, Star Formation, Ammonia, Astronomical Maps, Carbon Monoxide, Radio Telescopes

Scientific paper

The authors report molecular observations of a recently discovered CO outflow source NGC 2071-north in L1630. The data include 12CO, 13CO, and C18O spectra and NH3 spectra. The distribution of high-velocity CO wings indicates an extended outflow whose dynamical age is 1.7×105yr. The driving source of the outflow is an IRAS source having a luminosity of 40 L_sun;, which shows a far-infrared spectrum similar to T Tau. The outflow is associated with a small quiescent molecular cloud whose mass is 300 M_sun;. The outflow is shown to have kinetic energy comparable to that of the quiescent cloud.

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