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Spectroscopic Simulation of Diffuse Interstellar Lines and a Laboratory Model for Interstellar Chemical Synthesis

Published online by Cambridge University Press:  14 August 2015

F. M. Johnson ,
D. T. Bailey  and
P. A. Wegner
F. M. Johnson
Affiliation:
Dept. of Physics, California State University, Fullerton, Calif. 92634, U.S.A.
D. T. Bailey
Affiliation:
Dept. of Chemistry, California State University, Fullerton, Calif. 92634, U.S.A.
P. A. Wegner
Affiliation:
Dept. of Chemistry, California State University, Fullerton, Calif. 92634, U.S.A.

Abstract

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The interstellar existence of dipyridyl magnesium tetrabenzporphin (I) is supported by the spectroscopic coincidence of laboratory generated and astronomically observed diffuse interstellar lines. A potential route for the synthesis of I in space from molecules which exist or are expected to exist there will be discussed.

Type
Part VI Physical Processes, Theory and Experiment
Information
Symposium - International Astronomical Union , Volume 52: Interstellar Dust and Related Topics , 1973 , pp. 317 - 321
Copyright
Copyright © Reidel 1973 

References

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