A study of the noncollimation of C18O (J = 1-0) molecular outflows in Cepheus E.

Details A study of the noncollimation of C18O (J = 1-0) molecular outflows in Cepheus E. A study of the noncollimation of C18O (J = 1-0) molecular outflows in Cepheus E.

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998acasn..39..405y&link_type=abstract

Acta Astron. Sin., Vol. 39, No. 4, p. 405 - 411

Astronomy and Astrophysics

Astronomy

Molecular Clouds: Molecular Outflows

Scientific paper

The author studied the contour maps integrated over a 0.5 km/s velocity range from -11.5 to -9.0 km/s. It may be seen from the contour maps that the integrated intensity of C18O (J = 1-0) emission in the contour maps of the blue-shifted components relative to the peak velocity is larger than that of the red-shifted components. Meanwhile, the noncollimation of molecular outflows in integrated intensity maps is caused by the noncollimation of the blue-shifted components relative to the peak velocity.

Affiliated with

Also associated with

No associations

Rating

A study of the noncollimation of C18O (J = 1-0) molecular outflows in Cepheus E. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A study of the noncollimation of C18O (J = 1-0) molecular outflows in Cepheus E., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A study of the noncollimation of C18O (J = 1-0) molecular outflows in Cepheus E. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1073912