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New Detections of Spectral Lines in the Frequency Range 260-285 Ghz

Published online by Cambridge University Press:  14 August 2015

N. Erickson ,
J. H. Davis ,
N.J. Evans II ,
R. B. Loren ,
L. Mundy ,
W.L. Peters III ,
M. Scholtes  and
P.A. Vanden Bout
N. Erickson
Affiliation:
University of California-Berkeley
J. H. Davis
Affiliation:
University of Texas-Austin
N.J. Evans II
Affiliation:
University of Texas-Austin
R. B. Loren
Affiliation:
University of Texas-Austin
L. Mundy
Affiliation:
University of Texas-Austin
W.L. Peters III
Affiliation:
University of Texas-Austin
M. Scholtes
Affiliation:
University of Texas-Austin
P.A. Vanden Bout
Affiliation:
University of Texas-Austin

Extract

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The upper half of the frequency band lying between the atmospheric water lines at 183 and 323 GHz is virtually unexplored by spectroscopists of interstellar matter. The only published observations are those of Huggins et al. (1979) who detected the J=3-2 lines of HCN, HNC, and HCO+ in the Orion A molecular cloud (OMC-1). We report here the results of extensive observations made in March and April of 1979 with a University of California (Berkeley) receiver on the Texas 4.9-m antenna.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 25 - 30
Copyright
Copyright © Reidel 1980 

References

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