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High-resolution UVES/VLT spectra of white dwarfs observed for the ESO SN Ia Progenitor Survey. III. DA white dwarfs

机译:观察到EsO sN的白矮星的高分辨率UVEs / VLT光谱   Ia祖先调查。 III。 Da白矮星

摘要

The ESO Supernova Ia Progenitor Survey (SPY) took high-resolution spectra ofmore than 1000 white dwarfs and pre-white dwarfs. About two thirds of the starsobserved are hydrogen-dominated DA white dwarfs. Here we present a catalog anddetailed spectroscopic analysis of the DA stars in the SPY. Atmosphericparameters effective temperature and surface gravity are determined for normalDAs. Double-degenerate binaries, DAs with magnetic fields or dM companions, areclassified and discussed. The spectra are compared with theoretical modelatmospheres using a chi^2 fitting technique. Our final sample contains 615 DAs,which show only hydrogen features in their spectra, although some aredouble-degenerate binaries. 187 are new detections or classifications. We alsofind 10 magnetic DAs (4 new) and 46 DA+dM pairs (10 new).
机译:ESO超新星Ia祖先调查(SPY)采集了1000多个白矮星和预白矮星的高分辨率光谱。观测到的恒星中约有三分之二是氢为主的DA白矮星。在这里,我们介绍了SPY中DA星的目录和详细的光谱分析。确定了正常DA的大气参数有效温度和表面重力。对双简并二进制文件,具有磁场的DA或dM伴随物进行了分类和讨论。使用chi ^ 2拟合技术将光谱与理论模型大气进行比较。我们的最终样品包含615个DA,尽管有些是双简并二元,但它们在光谱中仅显示氢特征。 187是新的检测或分类。我们还找到了10个磁性DA(4个新)和46个DA + dM对(10个新)。

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