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Ultraviolet imaging telescope observations of the horizontal branch in M13

机译:紫外线成像望远镜对M13中水平分支的观测

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Images of the globular cluster M13 were obtained with the Ultraviolet Imaging Telescope (UIT) during the Astro-2 Spacelab mission. A total of 488 stars are detected in the UIT B5 filter centered at 1620 A. Of an Uncrowded sample of 247 stars, 232 are well correlated with ground-based Johnson V photometry, which was Provided by K. Montgomery (1995, private communication). A color-magnitude diagram, constructed from the (m_1620-V) color index and the M_1620 magnitude, shows a well-populated, blue horizontal branch extending to a temperature in excess of 35,000 K. A King plot of radial density distribution is satisfied by an exponential of index α=3.0, which is consistent with Laget et al.
机译:在Astro-2太空实验室任务期间,通过紫外线成像望远镜(UIT)获得了球状星团M13的图像。在以1620 A为中心的UIT B5滤镜中总共检测到488颗恒星。在247颗不拥挤的恒星样本中,有232颗与地面的Johnson V光度法密切相关,这是由K. Montgomery提供的(1995年,私人通讯) 。由(m_1620-V)颜色指数和M_1620幅度构成的色度图显示了一个分布良好的蓝色水平分支,延伸到超过35,000 K的温度。径向密度分布的King图满足指数为α= 3.0的指数,这与Laget等人一致。

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