Mira variables in globular clusters are used as a new, independent distance anchor, yielding a 3.7% Hubble constant of 73.06 ± 2.67 km/s/Mpc.
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Absolute Calibration of Cluster Mira Variables to Provide a New Anchor for the Hubble Constant Determination
Mira variables in globular clusters are used as a new, independent distance anchor, yielding a 3.7% Hubble constant of 73.06 ± 2.67 km/s/Mpc.