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References

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  1. A. A. Michelson and F. G. Pease, Astrophys. J. 53, 249–259 (1921).
    [CrossRef]

1921 (1)

A. A. Michelson and F. G. Pease, Astrophys. J. 53, 249–259 (1921).
[CrossRef]

Michelson, A. A.

A. A. Michelson and F. G. Pease, Astrophys. J. 53, 249–259 (1921).
[CrossRef]

Pease, F. G.

A. A. Michelson and F. G. Pease, Astrophys. J. 53, 249–259 (1921).
[CrossRef]

Astrophys. J. (1)

A. A. Michelson and F. G. Pease, Astrophys. J. 53, 249–259 (1921).
[CrossRef]

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Figures (2)

Fig. 1
Fig. 1

The arrows indicate the direction of the light rays converging from an objective. The broken lines that divide the components of the double prisms represent a semitransparent film of metal.

Fig. 2
Fig. 2

The arrows indicate the direction of rays from a distant source. As in Fig. 1 the broken lines signify a semitransparent film of metal.