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PSR J0952−0607: The Fastest and Heaviest Known Galactic Neutron Star

  • Authors: Roger W. Romani, D. Kandel, Alexei V. Filippenko, Thomas G. Brink, WeiKang Zheng

Roger W. Romani et al 2022 The Astrophysical Journal Letters 934 .

  • Provider: AAS Journals

Caption: Figure 3.

RV measurements for J0952. Dot size is proportional to the correlation coefficient R; low-significance correlations with R < 2 are marked with black crosses and are excluded from all fits. Three higher-significance points marked with green crosses appear as outliers and are optionally excluded for the “trimmed” fit. The background curve is the best-fit RV curve for the heating model fit to the light curve in Figure 1. The lower panel shows the fit residuals.

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