Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-23T19:32:07.629Z Has data issue: false hasContentIssue false
  • English
  • Français

High Velocity Co Wings in NGC 2071 and GL 490 Observed with the 45-m Telescope

Published online by Cambridge University Press:  04 August 2017

Y. Fukui ,
T. Iwata  and
T. Takano
Y. Fukui
Affiliation:
Nagoya University, Japan
T. Iwata
Affiliation:
Nagoya University, Japan
T. Takano
Affiliation:
University of Köln, Federal Republic of Germany

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have used the 45-m telescope for mapping two CO broad wing sources NGC 2071 and GL490 with a 15″ beam in the J = 1-0 line. We obtained 250 CO and 130 13CO spectra for NGC 2071 and 150 CO spectra for GL490. The observations were made with the highest angular resolution for the CO line and, as well, cover the whole extent of the outflows. The results reveal significant details of the angular distribution of the CO wings.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 328
Copyright
Copyright © Reidel 1987