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首页> 外文期刊>The Astrophysical Journal. Supplement Series >The R-Process Alliance: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo
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The R-Process Alliance: Fourth Data Release from the Search for R-process-enhanced Stars in the Galactic Halo

机译:R-Process Alliance:第四个数据从Galactic Halo中搜索R-Process-Conved Stars的搜索

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This compilation is the fourth data release from the R-Process Alliance (RPA) search for r-process-enhanced stars and the second release based on "snapshot" high-resolution (R similar to 30,000) spectra collected with the du Pont 2.5 m Telescope. In this data release, we propose a new delineation between the r-I and r-II stellar classes at [Eu Fe] = +0.7, instead of the empirically chosen [Eu Fe] = +1.0 level previously in use, based on statistical tests of the complete set of RPA data released to date. We also statistically justify the minimum level of [Eu/Fe] for definition of the r-I stars, [Eu/Fe] > +0.3. Redefining the separation between r-I and r-II stars will aid in the analysis of the possible progenitors of these two classes of stars and determine whether these signatures arise from separate astrophysical sources at all. Applying this redefinition to previous RPA data, the number of identified r-II and r-I stars changes to 51 and 121, respectively, from the initial set of data releases published thus far. In this data release, we identify 21 new r-II, 111 new r-I (plus 3 re-identified), and 7 new (plus 1 re-identified) limited-r stars out of a total of 232 target stars, resulting in a total sample of 72 new r-II stars, 232 new r-I stars, and 42 new limited-r stars identified by the RPA to date.
机译:这是R-Process Alliance(RPA)搜索R-Process增强恒星的第四次数据发布,也是基于杜邦2.5米望远镜收集的“快照”高分辨率(R类似于30000)光谱的第二次数据发布。在本次数据发布中,我们根据迄今发布的整套RPA数据的统计测试,提出了在[Eu Fe]=+0.7时,r-I和r-II恒星类别之间的新划分,而不是之前使用的经验选择[Eu Fe]=+1.0水平。我们还从统计学上证明了r-I星定义的最低[Eu/Fe]水平[Eu/Fe]>+0.3。重新定义r-I和r-II恒星之间的间隔将有助于分析这两类恒星的可能祖先,并确定这些特征是否来自单独的天体物理源。将这一重新定义应用于之前的RPA数据,识别出的r-II和r-I星的数量从迄今为止发布的最初数据集分别变为51和121。在本次数据发布中,我们在总共232颗目标星中识别出21颗新r-II星、111颗新r-I星(加上3颗重新识别)和7颗新(加上1颗重新识别)受限r星,从而得出迄今为止RPA识别的72颗新r-II星、232颗新r-I星和42颗新受限r星的总样本。

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