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Molecular Clouds near Supernova Remnants

Published online by Cambridge University Press:  14 August 2015

V. I. Slysh ,
T. L. Wilson ,
T. Pauls  and
C. Henkel
V. I. Slysh
Affiliation:
Space Research Institute, Academy of Science Profsojuznaja 88, 117810 Moscow, USSR
T. L. Wilson
Affiliation:
Max-Planck-Institut für Radioastronomie Auf dem Hügel 69, 5300 Bonn 1, FRG
T. Pauls
Affiliation:
Max-Planck-Institut für Radioastronomie Auf dem Hügel 69, 5300 Bonn 1, FRG
C. Henkel
Affiliation:
Max-Planck-Institut für Radioastronomie Auf dem Hügel 69, 5300 Bonn 1, FRG

Abstract

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A survey of 14 SNR's in the 4.8 GHz absorption line of H2CO shows that two of them, W28 and W44, possibly interact with molecular clouds. The interaction leads to acceleration of a part of the molecular cloud to a velocity of ∼5 km s-1 without a significant increase in the kinetic temperature or turbulence.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 473 - 478
Copyright
Copyright © Reidel 1980 

References

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