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首页> 外文期刊>The Astrophysical Journal. Supplement Series >Gaia RR Lyrae Stars in Nearby Ultra-faint Dwarf Satellite Galaxies
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Gaia RR Lyrae Stars in Nearby Ultra-faint Dwarf Satellite Galaxies

机译:盖亚rr leyrae星星在附近的超薄矮小卫星星系

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We search for RR Lyrae stars (RRLs) in 27 nearby (<100 kpc) ultra-faint dwarf satellite galaxies using the Gaia DR2 catalog of RRLs. Based on proper motions, magnitudes, and location on the sky, we associate 47 Gaia RRLs with 14 different satellites. Distances based on RRLs are provided for those galaxies. We have identified RRLs for the first time in the Tucana II dwarf galaxy, and find additional members in Ursa Major II, Coma Berenices, Hydrus I, Bootes I, and Bootes III. In addition we have identified candidate extra-tidal RRLs in six galaxies, which suggests they may be undergoing tidal disruption. We found 10 galaxies have no RRLs either in Gaia or in the literature. However, given the known completeness of Gaia DR2 we cannot conclude these galaxies indeed lack variable stars of this type.
机译:我们在附近的27位(<100 kPc)超薄矮小卫星卫星星系中搜索rr Lyrae Stars(RRL)使用RRLS的盖亚DR2目录。 基于天空的适当的动作,大小和位置,我们将47张Gaia RRL与14种不同的卫星联系起来。 基于RRL的距离为这些星系提供。 我们在Tucana II Dwarf Galaxy中首次识别了RRL,并在Ursa Major II,Coma Berenices,Hydrus I,靴子I和靴子III中找到其他成员。 此外,我们已经确定了六个星系中的候选人额外潮流,这表明他们可能正在发生潮汐中断。 我们发现10个星系在盖亚或文献中没有RRL。 然而,鉴于盖亚DR2的已知完整性,我们不能得出结论这些星系,确实缺少这种类型的可变星星。

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