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LONG-BASELINE INTERFEROMETRIC OBSERVATIONS OF CEPHEIDS

机译:头颅的长基线干涉观察

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摘要

We present observations of the Galactic Cepheids η Aql and ζ Gem. Our observations are able to resolve the diameter changes associated with pulsation. This allows us to determine the distance to the Cepheids independent of photometric observations. We determine a distance to η Aql of 320 +- 32 pc and a distance to ζ Gem of 362 +- 38 pc. These observations allow us to calibrate surface brightness relations for use in extraga-lactic distance determination. They also provide a measurement of the mean diameter of these Cepheids, which is useful in constructing structural models of this class of star.
机译:我们介绍了银河造父星ηAql和ζGem的观测结果。我们的观察结果能够解决与脉动相关的直径变化。这使我们能够确定与造父变星之间的距离,而与光度学观测无关。我们确定到ηAql的距离为320 +-32 pc,到ζGem的距离为362 +-38 pc。这些观察结果使我们能够校准表面亮度关系,以用于计外距离确定。他们还提供了这些造父变星的平均直径的测量值,这对于构建此类恒星的结构模型很有用。

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