Distances from the Correlation Between Galaxy Luminosities and Rotation Rates
作者： R. Brent Tully
DOI: 10.1007/978-94-011-4734-7_12
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摘要: A large luminosity-linewidth template sample is now available, improved absorption corrections have been derived, and there are a statistically significant number of galaxies with well determined distances to supply the zero point. revised estimate Hubble Constant H0 = 77±4 km s−1 Mpc−1 where error 95% probable statistical error. Systematic uncertainties potentially twice as large.
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