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Enigmas from the Sloan Digital Sky Survey DR7 White Dwarf Catalog

机译:来自Sloan Digital Sky Survey DR7 White Dwarf目录的谜

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We report results from a continuation of our searches for magnetic white dwarfs paired in a detached binary with a non-degenerate companion, using the Data Release 7 (DR7) of the Sloan Digital Sky Survey. Some 19,712 spectroscopically-identified white dwarfs from the Kleinman et al. paper were examined, including 1,951 white dwarf - M dwarf pairs. The polar (AM Her) system ST LMi in a low state was found but later recognized not to be a detached pair. Our basic result is that the original situation reported 10 years ago is still the case with now very high statistical significance. Detached polar progenitors, apart from Low Accretion Rate Polars (LARPs), are not found. Magnetic white dwarfs likely form from mergers of (nonmagnetic) white dwarfs, while polars and intermediate polars emerge from common envelope evolution as close binaries - either Roche-lobe-filling mass transfer mode or LARPs.
机译:我们通过使用Sloan Digital Sky调查的数据版本7(DR7)在分离的二进制中,在与非退化伴侣中携带的磁性白矮星的延续报告结果报告。来自Kleinman等人的一些19,712个光谱识别的白矮星。检查纸张,包括1,951个白矮星 - M矮人对。发现低状态的极性(AM)系统ST LMI,但后来识别不作为拆卸对。我们的基本结果是,10年前报告的原始情况仍然是现在非常高的统计显着性。除了低积累率波兰(LARP),分离的极性祖细胞潜水剂未被发现。磁性白矮星可能从(非磁性)白矮星的合并,而波拉和中间点从普通的信封演变中出现,作为近二进制 - 罗氏 - 填充质量传递模式或碱度。

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