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Amplification and Absorption of the 9 cm2Π, J = ½ A-Doublet Lines of Interstellar CH

  • F. F. Gardner (a1) and B. J. Robinson (a1)

Extract

Following the detection of the 9 cm ground-state triplet of CH by Rydbeck et al. (1973), preliminary observations at the CH frequencies were made with the Parkes 64-m telescope (beamwidth ∼6′ arc) in December 1973 and January 1974. We have detected the CH lines in many galactic HII regions and in the direction of the galactic centre.

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Manchester, R. N., Robinson, B. J., and Goss, W. M., Aust. J. Phys., 23, 751 (1970).
Robinson, B. J., 1974, Proc. IAU Symp. No. 60 on ‘Galactic Radio Astronomy’ (in press).
Robinson, B. J., Gardner, F. F., Sinclair, M. W., and Whiteoak, J. B., Nature, 248, 31,(1974).
Rydbeck, O. E. H., Ellder, J., and Irvine, W. M., Nature, 246, 466 (1973).
Rydbeck, O. E. H., Ellder, J., Irvine, W. M., Sume, A., and Hjalmarson, Å., Astron. Astrophys. (in press) (1974).
Shaver, P. A., and Goss, W. M., Aust. J. Phys. Astrophys. Suppl.. No. 14, 133 (1970).

Amplification and Absorption of the 9 cm2Π, J = ½ A-Doublet Lines of Interstellar CH

  • F. F. Gardner (a1) and B. J. Robinson (a1)

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