A New Cepheid Distance to the Maser-Host Galaxy NGC 4258 and Its Implications for the Hubble Constant
We present initial results from a time series BVI survey of two fields in NGC 4258 using the HST ACS. This galaxy was selected because of its accurate maser-based distance, which is anticipated to have a total uncertainty of 63%. The goal of the HST observations is to provide an absolute calibration...
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Veröffentlicht in: | The Astrophysical journal 2006-12, Vol.652 (2), p.1133-1149 |
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