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- W1992619985 abstract "Recently, statistical correlations were found between near-infrared luminosities and ring sizes in field resonance-ringed galaxies. These correlations are proposed as a new class of tertiary distance indicators in the nearby universe (where redshifts ≲30, 000kms−1). The most suitable application of the indicators will be to measure the Hubble constant. Detailed formulae are derived to evaluate distances to field ringed galaxies and H0, as well as the error levels involved in using this method. Numerical simulations show that through the measurements of over a thousand nearby ringed galaxies the method can yield a value of H0 with its root-mean-square random error within ≈6% and systematic error most likely below ≈10% (excluding the systematic error due to other indicators that are used to calibrate the correlations). Future such measurements should help to check the H0 values from conventional methods." @default.
- W1992619985 created "2016-06-24" @default.
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- W1992619985 date "2009-02-12" @default.
- W1992619985 modified "2023-09-23" @default.
- W1992619985 title "RESONANCE RINGS IN GALAXIES AS NEW TERTIARY DISTANCE INDICATORS" @default.
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- W1992619985 doi "https://doi.org/10.1088/0004-6256/137/3/3455" @default.
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