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arXiv 1808.03243astro-ph.SR
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来自新Luyten十分之二星表的四个新的食中M矮星系统

Four new eclipsing mid M-dwarf systems from the New Luyten Two Tenths catalog

Jonathan M. Irwin, David Charbonneau, Gilbert A. Esquerdo, David W. Latham, Jennifer G. Winters, Jason A. Dittmann, Elisabeth R. Newton, Zachory K. Berta-Thomps… 展开作者

Jonathan M. Irwin, David Charbonneau, Gilbert A. Esquerdo, David W. Latham, Jennifer G. Winters, Jason A. Dittmann, Elisabeth R. Newton, Zachory K. Berta-Thompson, Perry Berlind, Michael L. Calkins

摘要:

利用MEarth-北和MEarth-南过境调查的数据,我们提出了四个中M矮星系统的日食检测:LP 107-25,LP 261-75,LP 796-24和LP 991-15。结合MEarth测光和光谱跟踪观测,我们发现LP 107-25和LP 796-24是短周期(分别为1.388和0.523天)的食双星,在三线系统中有大量的第三光污染来自遥远的同伴。LP 261-75是一个短周期(1.882天)单线系统,由一颗中M矮星和另一颗远距离可见棕矮星伴星组成。LP 991-15是一颗长周期(29.3天)双线食双星,在偏心轨道上运行,其几何形状只产生主食。给出了LP 991-15的光谱轨道,以及LP 107-25和LP 261-75的初始轨道。

英文摘要:

Using data from the MEarth-North and MEarth-South transit surveys, we present the detection of eclipses in four mid M-dwarf systems: LP 107-25, LP 261-75, LP 796-24, and LP 991-15. Combining the MEarth photometry with spectroscopic follow-up observations, we show that LP 107-25 and LP 796-24 are short-period (1.388 and 0.523 day, respectively) eclipsing binaries in triple-lined systems with substantial third light contamination from distant companions. LP 261-75 is a short-period (1.882 day) single-lined system consisting of a mid M-dwarf eclipsed by a probable brown dwarf secondary, with another distant visual brown dwarf companion. LP 991-15 is a long-period (29.3 day) double-lined eclipsing binary on an eccentric orbit with a geometry which produces only primary eclipses. A spectroscopic orbit is given for LP 991-15, and initial orbits for LP 107-25 and LP 261-75.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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