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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

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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

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Roh, D.G., Kim, H.R., Minh, Y.C., Auh, B.R. and Koo, B.C. 1991, in preparation.Google Scholar