Abstract

The relative gf-values of 256 lines in 58 multiplets in the spectrum of Co i have been measured in electric furnace absorption spectra. The lines lie in the wavelength range 2987–6450 A and arise from low terms whose excitation potentials are between 0.00 and 3.24 ev.

© 1955 Optical Society of America

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References

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  1. R. B. King and A. S. King, Astrophys. J. 87, 24 (1938); W. W. Carter, Phys. Rev. 76, 962 (1949).
    [Crossref]
  2. R. B. King, Astrophys. J. 94, 27 (1941).
    [Crossref]
  3. R. B. King, Astrophys. J. 105, 376 (1947).
    [Crossref]
  4. R. B. King, Astrophys. J. 108, 87 (1948).
    [Crossref]
  5. A. J. Hill and R. B. King, J. Opt. Soc. Am. 41, 315 (1951).
    [Crossref]
  6. A. S. King, Astrophys. J. 56, 318 (1922).
    [Crossref]
  7. P. Schulz, Ann. Physik 1, 107 (1947).
    [Crossref]
  8. W. A. Baum and W. L. Dunkelman, J. Opt. Soc. Am. 40, 782 (1950).
    [Crossref]
  9. The equivalent width of an absorption line is defined as the number of angstrom units of the continuous spectrum totally absorbed by the integrated absorption in the line.
  10. Contributions from the Princeton University Observatory, No.  20 (1945).
  11. If reference 10 is not available the term designations of all lines in Table I may be found in the term analysis of Co i given by Russell, King, and Moore, Phys. Rev. 58, 407 (1940).
    [Crossref]

1951 (1)

1950 (1)

1948 (1)

R. B. King, Astrophys. J. 108, 87 (1948).
[Crossref]

1947 (2)

R. B. King, Astrophys. J. 105, 376 (1947).
[Crossref]

P. Schulz, Ann. Physik 1, 107 (1947).
[Crossref]

1945 (1)

Contributions from the Princeton University Observatory, No.  20 (1945).

1941 (1)

R. B. King, Astrophys. J. 94, 27 (1941).
[Crossref]

1940 (1)

If reference 10 is not available the term designations of all lines in Table I may be found in the term analysis of Co i given by Russell, King, and Moore, Phys. Rev. 58, 407 (1940).
[Crossref]

1938 (1)

R. B. King and A. S. King, Astrophys. J. 87, 24 (1938); W. W. Carter, Phys. Rev. 76, 962 (1949).
[Crossref]

1922 (1)

A. S. King, Astrophys. J. 56, 318 (1922).
[Crossref]

Baum, W. A.

Dunkelman, W. L.

Hill, A. J.

King,

If reference 10 is not available the term designations of all lines in Table I may be found in the term analysis of Co i given by Russell, King, and Moore, Phys. Rev. 58, 407 (1940).
[Crossref]

King, A. S.

R. B. King and A. S. King, Astrophys. J. 87, 24 (1938); W. W. Carter, Phys. Rev. 76, 962 (1949).
[Crossref]

A. S. King, Astrophys. J. 56, 318 (1922).
[Crossref]

King, R. B.

A. J. Hill and R. B. King, J. Opt. Soc. Am. 41, 315 (1951).
[Crossref]

R. B. King, Astrophys. J. 108, 87 (1948).
[Crossref]

R. B. King, Astrophys. J. 105, 376 (1947).
[Crossref]

R. B. King, Astrophys. J. 94, 27 (1941).
[Crossref]

R. B. King and A. S. King, Astrophys. J. 87, 24 (1938); W. W. Carter, Phys. Rev. 76, 962 (1949).
[Crossref]

Moore,

If reference 10 is not available the term designations of all lines in Table I may be found in the term analysis of Co i given by Russell, King, and Moore, Phys. Rev. 58, 407 (1940).
[Crossref]

Russell,

If reference 10 is not available the term designations of all lines in Table I may be found in the term analysis of Co i given by Russell, King, and Moore, Phys. Rev. 58, 407 (1940).
[Crossref]

Schulz, P.

P. Schulz, Ann. Physik 1, 107 (1947).
[Crossref]

Ann. Physik (1)

P. Schulz, Ann. Physik 1, 107 (1947).
[Crossref]

Astrophys. J. (5)

R. B. King and A. S. King, Astrophys. J. 87, 24 (1938); W. W. Carter, Phys. Rev. 76, 962 (1949).
[Crossref]

R. B. King, Astrophys. J. 94, 27 (1941).
[Crossref]

R. B. King, Astrophys. J. 105, 376 (1947).
[Crossref]

R. B. King, Astrophys. J. 108, 87 (1948).
[Crossref]

A. S. King, Astrophys. J. 56, 318 (1922).
[Crossref]

Contributions from the Princeton University Observatory (1)

Contributions from the Princeton University Observatory, No.  20 (1945).

J. Opt. Soc. Am. (2)

Phys. Rev. (1)

If reference 10 is not available the term designations of all lines in Table I may be found in the term analysis of Co i given by Russell, King, and Moore, Phys. Rev. 58, 407 (1940).
[Crossref]

Other (1)

The equivalent width of an absorption line is defined as the number of angstrom units of the continuous spectrum totally absorbed by the integrated absorption in the line.

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Tables (1)

Tables Icon

Table I Relative gf-values for lines of Co i.