Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-25T12:36:31.954Z Has data issue: false hasContentIssue false
  • English
  • Français

Molecular Line Observations Towards W58 and GL490

Published online by Cambridge University Press:  07 August 2017

D.G. Roh ,
H.R. Kim ,
Y.C. Minh ,
B.R. Auh  and
B.C. Koo
D.G. Roh
Affiliation:
Radio Astronomy Section Institute of Space Science and Astronomy, Korea
H.R. Kim
Affiliation:
Radio Astronomy Section Institute of Space Science and Astronomy, Korea
Y.C. Minh
Affiliation:
Radio Astronomy Section Institute of Space Science and Astronomy, Korea
B.R. Auh
Affiliation:
Radio Astronomy Section Institute of Space Science and Astronomy, Korea
B.C. Koo
Affiliation:
Harvard-Smithsonian Center for Astrophysics, U.S.A.

Abstract

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 observed 3 mm transitions of several interstellar molecules toward star-forming regions in W58 and GL490 using the 14 m Daeduk Radio Telescope (Korea). We derive molecular abundances for the“broad” components observed with a high spectral resolution, which could represent the abundances of outflowing materials.

Type
Quiescent Clouds and Regions of Star Formation
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 225 - 226
Copyright
Copyright © Kluwer 1992 

References

REFERENCE:

van Gorkom, J.H. 1981, A. & Ap. , 94, 259.Google Scholar
Israel, F.P. 1980, Ap.J. , 236, 465.Google Scholar
Mundy, L.G. and Adelman, G.A. 1988, Ap.J. , 329, 907.Google Scholar
Roh, D.G., Kim, H.R., Minh, Y.C., Auh, B.R. and Koo, B.C. 1991, in preparation.Google Scholar