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Observations of the 89 GHz Transition of HCO+ in Orion

Published online by Cambridge University Press:  25 April 2016

R. A. Batchelor ,
M. G. McCulloch  and
J. B. Whiteoak
R. A. Batchelor
Affiliation:
Division of Radiophysics, CSIRO, Sydney
M. G. McCulloch
Affiliation:
Division of Radiophysics, CSIRO, Sydney
J. B. Whiteoak
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

Observations of CO emission (Kutner et al. 1977) have delineated a molecular cloud extending over several square degrees in the Orion region, and extensive surveys have been made of several other molecules (e.g. CN, CS, HCN, H2CO, H2H+) in the densest regions of this cloud.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 1 , 1980 , pp. 98 - 100
Copyright
Copyright © Astronomical Society of Australia 1980

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References

Cole, T. W., and Milne, D. K., Proc. Astron. Soc. Aust., 3, 1 (1977).Google Scholar
Gardner, F. F., Batchelor, R. A., McCulloch, M. G., Simons, L. W., and Whiteoak, J. B., Proc. Astron. Soc. Aust., 3, 264 (1978).Google Scholar
Gatley, I., Becklin, E. E., Matthews, K., Neugebauer, G., Penston, M. V., and Scoville, N., Astrophys. J., 191, L121 (1974).CrossRefGoogle Scholar
Gottlieb, C. A., and Ball, J. A., Astrophys. J., 184, L59 (1973).CrossRefGoogle Scholar
Huggins, P. J., Phillips, T. G., Neugebauer, G., Werner, M. W., Wannier, P. G., and Ennis, D., Astrophys. J., III, 441 (1979).Google Scholar
Kutner, M. L., Evans, N. J., and Tucker, K. D., Astrophys. J., 209, 452 (1976).Google Scholar
Kutner, M. L., Tucker, K. D., Chin, G., and Thaddeus, P., Astrophys. J., 215, 521 (1977).Google Scholar
Liszt, H. S., Wilson, R. W., Penzias, A. A., Jefferts, K. B., Wannier, P. G., and Solomon, P. M., Astrophys. J., 190, 557 (1974).CrossRefGoogle Scholar
Snyder, L. E., Watson, W. D., and Hollis, J. M., Astrophys. J., III, 79 (1977).CrossRefGoogle Scholar
Snyder, L. E., Hollis, J. M., Lovas, F. J., and Ulich, B. L., Astrophys. J., 209, 67 (1976).Google Scholar
Turner, B. E., and Thaddeus, P., Astrophys. J., 211, 755 (1977).Google Scholar
Watson, W. D., Rev. Mod. Phys., 48, 513 (1976).Google Scholar
Whiteoak, J. B., and Gardner, F. F., Mon. Not. R. Astron. Soc., 185, 33P (1978).Google Scholar
Woods, R. C., Dixon, T. A., Saykally, R. J., and Szanto, P. G., Phys. Rev. Lett., 35, 1269 (1975).Google Scholar