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References

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  1. Astrophys. J.,  35, p. 237, 1912; and Astrophys. J.,  48, p. 65, 1918.
    [Crossref]
  2. Proc. Roy. Soc., 88, p. 404.
  3. Phys. Rev., 25, p. 433.
  4. Bul. Bur. Std.14, p. 167.
  5. See Hayes, Am. Jour. Psych.,  22, p. 369, case M.S. This opinion is also supported by Prof. Dunlap of Johns Hopkins.

1912 (1)

Astrophys. J.,  35, p. 237, 1912; and Astrophys. J.,  48, p. 65, 1918.
[Crossref]

Hayes,

See Hayes, Am. Jour. Psych.,  22, p. 369, case M.S. This opinion is also supported by Prof. Dunlap of Johns Hopkins.

Am. Jour. Psych. (1)

See Hayes, Am. Jour. Psych.,  22, p. 369, case M.S. This opinion is also supported by Prof. Dunlap of Johns Hopkins.

Astrophys. J. (1)

Astrophys. J.,  35, p. 237, 1912; and Astrophys. J.,  48, p. 65, 1918.
[Crossref]

Other (3)

Proc. Roy. Soc., 88, p. 404.

Phys. Rev., 25, p. 433.

Bul. Bur. Std.14, p. 167.

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Figures (4)

Fig. 1
Fig. 1

Equal-area luminosity curves (Source at 2045 °K).

Fig. 2
Fig. 2

Visibility functions derived from the luminosity curves of Fig. 1.

Fig. 3
Fig. 3

Visibility thresholds.

Fig. 4
Fig. 4

Detail of Fig. 3.