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The Extragalactic Distance Scale Key Project XVIII. The Discovery of Cepheids and a New Distance to NGC 4535 Using the Hubble Space Telescope

机译:河外距离量表重点项目XVIII。发现  造父变星与NGC 4535的新距离使用哈勃太空望远镜

摘要

We report on the discovery of Cepheids in the Virgo spiral galaxy NGC 4535,based on observations made with the Wide Field and Planetary Camera 2 on boardthe Hubble Space Telescope. NGC 4535 is one of 18 galaxies observed as a partof The HST Key Project on the Extragalactic Distance Scale which aims tomeasure the Hubble constant to 10% accuracy. NGC 4535 was observed over 13epochs using the F555W filter, and over 9 epochs using the F814W filter. TheHST F555W and F814W data were transformed to the Johnson V and Kron-Cousins Imagnitude systems, respectively. Photometry was performed using two independentprograms, DoPHOT and DAOPHOT II/ALLFRAME. Period-luminosity relations in the V and I bands were constructed using 39high-quality Cepheids present in our set of 50 variable candidates. We obtain adistance modulus of 31.02+/-0.26 mag, corresponding to a distance of 16.0+/-1.9Mpc. Our distance estimate is based on values of mu = 18.50 +/- 0.10 mag andE(V-I) = 0.13 mag for the distance modulus and reddening of the LMC,respectively.
机译:我们基于哈勃太空望远镜在宽视场和行星照相机2上所做的观测,报告了在处女座旋涡星系NGC 4535中发现造父变星的情况。 NGC 4535是作为HST关键项目“银河外距离尺度”观测到的18个星系之一,该计划旨在将哈勃常数测量到10%的精度。使用F555W滤镜观察到NGC 4535超过13个历元,而使用F814W滤镜观察到超过9个历元。 HST F555W和F814W数据分别转换为Johnson V和Kron-Cousins Imagnitude系统。使用两个独立的程序DoPHOT和DAOPHOT II / ALLFRAME进行测光。 V和I波段的周期光度关系是使用我们的50个变量候选集中存在的39个高质量造父变星构建的。我们获得31.02 +/- 0.26 mag的距离模量,对应于16.0 +/- 1.9Mpc的距离。我们的距离估算分别基于mu = 18.50 +/- 0.10 mag和E(V-I)= 0.13 mag的距离模量和LMC的发红。

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