Hostname: page-component-745bb68f8f-l4dxg Total loading time: 0 Render date: 2025-01-08T13:54:53.981Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Clark, F.O., Brown, R.D., Godfrey, P.D., Storey, J.W.V., and Johnson, D.R.: 1976, Astrophys. J. (Letters), 210, pp. L139-L140.Google Scholar
Erickson, N.R.: 1977, IEEE Trans. Microwave Theory and Tech., MTT-25, pp. 865-866.Google Scholar
Evans, N.J. II, Plambeck, R.L., and Davis, J.H.: 1979, Astrophys. J. (Letters) 227, pp. L25-L28.Google Scholar
Gottlieb, C.A., Lada, C.J., Gottlieb, E.W., Lilley, A.E., and Litvak, M.M.: 1975, Astrophys. J. 202, pp. 655-672.Google Scholar
Green, S.: 1975, Astrophys. J. 201, pp. 366-372.CrossRefGoogle Scholar
Huggins, P.J., Phillips, T.G., Neugebauer, G., Werner, M.W., Wannier, P.G., and Ennis, D.: 1979, Astrophys. J. 227, pp. 441-445.Google Scholar
Morris, M., Snell, R.L., and Vanden Bout, P.A.: 1977, Astrophys. J. 216, pp. 738-746.CrossRefGoogle Scholar
Penzias, A.A., and Burrus, C.A.: 1973, Ann. Rev. Astron. Astrophys. 11, pp. 51-72.Google Scholar
Snell, R.L., and Wootten, H.A.: 1979, Astrophys. J. 228, pp. 748-754.Google Scholar
Turner, B.E., and Thaddeus, P.: 1977, Astrophys. J. 211, pp. 755-771.Google Scholar
Wannier, P.G., and Linke, R.A.: 1978, Astrophys. J. 226, pp. 817-823.CrossRefGoogle Scholar