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  1. E. H. Pinnington, J. A. Kernahan, and C. C. Lin, Astrophys. J. 161. 339 (1970).
  2. K. O. Wright, E. K. Lee, T. V. Jacobson, and J. L. Greenstein, Publ. Dominion Astrophys. Observatory, Victoria 12, No. 7, 194 (1964).
  3. A. B. Underhill, Publ. Dominion Astrophys. Observatory, Victoria 11, Nos. 8, 225 and 15, 298 (1960).
  4. J. A. Kernahan, C. C. Lin, and E. H. Pinnington, J. Opt. Soc. Am. 60, 986 (1970).
  5. E. H. Pinnington and C. C. Lin, J. Opt. Soc. Am. 59, 717 (1969).
  6. M. R. Lewis, F. S. Zimnoch, and G. W. Wares, Phys. Rev. 178, 49 (1969).
  7. M. Druetta and M. C. Poulizac, Phys. Letters 29A, 651 (1969).
  8. H. E. White and A. Y. Eliason, Phys. Rev. 44, 753 (1933).
  9. We did not make observations at 2494 or 2517 Å. Our original reason for recording at 2510 Å was to check for the presence of the impurity C II line at this wavelength that we have observed in previous experiments.10 The possibility that O III lines could also occur in this region came to light only during the analysis of the data. For reasons given elsewhere,1 we have decided that O2+ ions formed the only significant component of the beam that struck the carbon foil. (The radiative lifetime of the C II line at 2510 Å is much shorter10 than the mean value of 3.6 nsec that we have observed for the line at 2510 Å in the present experiment.)
  10. E. H. Pinnington and C. C. Lin, J. Opt. Soc. Am. 59, 780 (1969).
  11. M. Druetta, private communication, 1970.
  12. W. L. Wiese, M. W. Smith, and B. M. Glennon, Atomic Transition Probabilities, Vol. 1, Natl. Bur. Std. (U. S.) NSRDS-NBS 4 (U. S. Govt. Printing Office, Washington, D. C., 1966).

Druetta, M.

M. Druetta and M. C. Poulizac, Phys. Letters 29A, 651 (1969).

M. Druetta, private communication, 1970.

Eliason, A. Y.

H. E. White and A. Y. Eliason, Phys. Rev. 44, 753 (1933).

Glennon, B. M.

W. L. Wiese, M. W. Smith, and B. M. Glennon, Atomic Transition Probabilities, Vol. 1, Natl. Bur. Std. (U. S.) NSRDS-NBS 4 (U. S. Govt. Printing Office, Washington, D. C., 1966).

Greenstein, J. L.

K. O. Wright, E. K. Lee, T. V. Jacobson, and J. L. Greenstein, Publ. Dominion Astrophys. Observatory, Victoria 12, No. 7, 194 (1964).

Jacobson, T. V.

K. O. Wright, E. K. Lee, T. V. Jacobson, and J. L. Greenstein, Publ. Dominion Astrophys. Observatory, Victoria 12, No. 7, 194 (1964).

Kernahan, J. A.

J. A. Kernahan, C. C. Lin, and E. H. Pinnington, J. Opt. Soc. Am. 60, 986 (1970).

Lee, E. K.

K. O. Wright, E. K. Lee, T. V. Jacobson, and J. L. Greenstein, Publ. Dominion Astrophys. Observatory, Victoria 12, No. 7, 194 (1964).

Lewis, M. R.

M. R. Lewis, F. S. Zimnoch, and G. W. Wares, Phys. Rev. 178, 49 (1969).

Lin, C. C.

E. H. Pinnington and C. C. Lin, J. Opt. Soc. Am. 59, 717 (1969).

J. A. Kernahan, C. C. Lin, and E. H. Pinnington, J. Opt. Soc. Am. 60, 986 (1970).

E. H. Pinnington and C. C. Lin, J. Opt. Soc. Am. 59, 780 (1969).

Pinnington, E. H.

E. H. Pinnington and C. C. Lin, J. Opt. Soc. Am. 59, 780 (1969).

J. A. Kernahan, C. C. Lin, and E. H. Pinnington, J. Opt. Soc. Am. 60, 986 (1970).

E. H. Pinnington and C. C. Lin, J. Opt. Soc. Am. 59, 717 (1969).

E. H. Pinnington, J. A. Kernahan, and C. C. Lin, Astrophys. J. 161. 339 (1970).

Poulizac, M. C.

M. Druetta and M. C. Poulizac, Phys. Letters 29A, 651 (1969).

Smith, M. W.

W. L. Wiese, M. W. Smith, and B. M. Glennon, Atomic Transition Probabilities, Vol. 1, Natl. Bur. Std. (U. S.) NSRDS-NBS 4 (U. S. Govt. Printing Office, Washington, D. C., 1966).

Underhill, A. B.

A. B. Underhill, Publ. Dominion Astrophys. Observatory, Victoria 11, Nos. 8, 225 and 15, 298 (1960).

Wares, G. W.

M. R. Lewis, F. S. Zimnoch, and G. W. Wares, Phys. Rev. 178, 49 (1969).

White, H. E.

H. E. White and A. Y. Eliason, Phys. Rev. 44, 753 (1933).

Wiese, W. L.

W. L. Wiese, M. W. Smith, and B. M. Glennon, Atomic Transition Probabilities, Vol. 1, Natl. Bur. Std. (U. S.) NSRDS-NBS 4 (U. S. Govt. Printing Office, Washington, D. C., 1966).

Wright, K. O.

K. O. Wright, E. K. Lee, T. V. Jacobson, and J. L. Greenstein, Publ. Dominion Astrophys. Observatory, Victoria 12, No. 7, 194 (1964).

Zimnoch, F. S.

M. R. Lewis, F. S. Zimnoch, and G. W. Wares, Phys. Rev. 178, 49 (1969).

Other (12)

E. H. Pinnington, J. A. Kernahan, and C. C. Lin, Astrophys. J. 161. 339 (1970).

K. O. Wright, E. K. Lee, T. V. Jacobson, and J. L. Greenstein, Publ. Dominion Astrophys. Observatory, Victoria 12, No. 7, 194 (1964).

A. B. Underhill, Publ. Dominion Astrophys. Observatory, Victoria 11, Nos. 8, 225 and 15, 298 (1960).

J. A. Kernahan, C. C. Lin, and E. H. Pinnington, J. Opt. Soc. Am. 60, 986 (1970).

E. H. Pinnington and C. C. Lin, J. Opt. Soc. Am. 59, 717 (1969).

M. R. Lewis, F. S. Zimnoch, and G. W. Wares, Phys. Rev. 178, 49 (1969).

M. Druetta and M. C. Poulizac, Phys. Letters 29A, 651 (1969).

H. E. White and A. Y. Eliason, Phys. Rev. 44, 753 (1933).

We did not make observations at 2494 or 2517 Å. Our original reason for recording at 2510 Å was to check for the presence of the impurity C II line at this wavelength that we have observed in previous experiments.10 The possibility that O III lines could also occur in this region came to light only during the analysis of the data. For reasons given elsewhere,1 we have decided that O2+ ions formed the only significant component of the beam that struck the carbon foil. (The radiative lifetime of the C II line at 2510 Å is much shorter10 than the mean value of 3.6 nsec that we have observed for the line at 2510 Å in the present experiment.)

E. H. Pinnington and C. C. Lin, J. Opt. Soc. Am. 59, 780 (1969).

M. Druetta, private communication, 1970.

W. L. Wiese, M. W. Smith, and B. M. Glennon, Atomic Transition Probabilities, Vol. 1, Natl. Bur. Std. (U. S.) NSRDS-NBS 4 (U. S. Govt. Printing Office, Washington, D. C., 1966).

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