Figure 3 from RELATIVISTIC MEASUREMENTS FROM TIMING THE BINARY PULSAR PSR B1913+16

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RELATIVISTIC MEASUREMENTS FROM TIMING THE BINARY PULSAR PSR B1913+16

Authors: J. M. Weisberg, and Y. Huang

2016 The Astrophysical Journal 829 55.

Provider: AAS Journals

Caption: Figure 3.

Orbital decay of PSR B1913+16 as a function of time. The curve represents the orbital phase shift expected from gravitational wave emission according to General Relativity. The points, with error bars too small to show, represent our measurements.

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