The noncollimation of molecular outflow and velocity components of C18O (J = 1-0) in Cepheus E.

Details The noncollimation of molecular outflow and velocity components of C18O (J = 1-0) in Cepheus E. The noncollimation of molecular outflow and velocity components of C18O (J = 1-0) in Cepheus E.

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999acaps..19...63y&link_type=abstract

Acta Astrophys. Sin., Vol. 19, No. 1, p. 63 - 67

Astronomy and Astrophysics

Astrophysics

Molecular Clouds: Molecular Outflows, Molecular Clouds: Velocity Distribution

Scientific paper

An analysis of the velocity-position maps of C18O (J = 1-0) in Cepheus E has revealed that the red-shifted component (relative to peak velocity) is distributed in the central core, while the blue-shifted component (relative to peak velocity) is distributed in the outflows towards the east and the northwest, as well as in the central core. This indicates that the noncollimation of molecular outflow in the integrated intensity map is caused by the noncollimation of the blue-shifted component.

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