作者: Thomas G. Barnes
DOI: 10.1063/1.3246527
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摘要: This review examines progress on the Pop I, fundamental‐mode Cepheid distance scale with emphasis recent developments in geometric and quasi‐geometric techniques for determination. Specifically I examine surface brightness method, interferometric pulsation trigonometric measurements. The three are found to be excellent agreement measures Galaxy. velocity p‐factor is of crucial importance first two these methods. A comparison determinations Cepheids demonstrates that observational p theoretical predictions agree within their uncertainties Galactic Cepheids.