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Effects of the UV radiation on the surrounding gas and dust

Published online by Cambridge University Press:  03 August 2017

A. Fuente ,
J. Martin-Pintado ,
J. Cernicharo ,
N. Brouillet  and
G. Duvert
A. Fuente
Affiliation:
Centro Astronómico de Yebes.Apdo. 148. E-19080 Guadalajara(Spain)
J. Martin-Pintado
Affiliation:
Centro Astronómico de Yebes.Apdo. 148. E-19080 Guadalajara(Spain)
J. Cernicharo
Affiliation:
Centro Astronómico de Yebes. Apdo. 148. E-19080 Guadalajara(Spain) IRAM. Divina Pastora, 7. E-18012 Granada(Spain)
N. Brouillet
Affiliation:
Observ. de Bordeaux, B.P. 21, F-33270 Floirac(France)
G. Duvert
Affiliation:
Observ. de Grenoble, B.P. 68, F-38402 Saint-Martin-d'Heres Cedex(France)

Abstract

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Two molecular clouds associated with well known reflection nebulosities have been studied in order to stablish the effects of the UV radiation on the surrounding gas and dust. Observations of the J=2 →1 and J=1 →0 transitions of CO and 13CO have been carried out with the telescopes POM 1 and POM 2 towards the clouds associated with LKHα 198 and HD200775. The IRAS maps at 12, 25, 60 and 100 μm towards these globules have been also examined.

Type
Poster Sessions
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 409 - 410
Copyright
Copyright © Kluwer 1991 

References

Fuente, A., Martín-Pintado, J., Cernicharo, J., Bachiller, R.: 1990, in press (to be published in Astron. Astrophys.)Google Scholar