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Leavitt: the period-brightness relation in Magellanic Cloud variables

Identified a strong relation between pulsation period and brightness among variable stars in the Small Magellanic Cloud.

What is recorded here?

Identified a strong relation between pulsation period and brightness among variable stars in the Small Magellanic Cloud.

Source-linked catalogue note. A detailed explanatory guide has not yet been prepared for this entry.

Scientific scope

The record concerns Leavitt’s analysis prepared for the 1912 Harvard circular; later calibration and distance-scale applications are separate.

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People and systems

Henrietta S. Leavitt

The named authors contributed to this scoped work; individual effort shares and later applications are not assigned by the byline.

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English catalogue narrative

Leavitt: the period-brightness relation in Magellanic Cloud variables

Identified a strong relation between pulsation period and brightness among variable stars in the Small Magellanic Cloud.

Scientific scope

The record concerns Leavitt’s analysis prepared for the 1912 Harvard circular; later calibration and distance-scale applications are separate.

Reading status

This is a source-linked WRS catalogue note. A full explanatory guide and independent scientific reconstruction have not been completed for this entry. Read the identified original work for its complete narrative and arguments.

People and systems

Henrietta S. Leavitt

The named authors contributed to this scoped work; individual effort shares and later applications are not assigned by the byline.

Original sources