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A Radial velocity survey of spatially resolved young, low-mass binaries ?

机译:对空间分辨的年轻低质量二进制文件进行的径向速度调查

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The identification and characterisation of low-mass binaries is of importance for a range of astrophysical investigations. Low-mass binaries in young (~10–100 Myr) moving groups (YMGs) in the solar neighborhood are of particular significance as they provide unique opportunities to calibrate stellar models and evaluate the ages and coevality of the groups themselves. Low-mass M-dwarfs have pre-main sequence life times on the order of ~100 Myr and therefore are continually evolving along a mass-luminosity track throughout the YMG phase, providing ideal laboratories for precise isochronal dating, if a model-independent dynamical mass can be measured. AstraLux lucky imaging multiplicity surveys have recently identified hundreds of new YMG low-mass binaries, where a subsample of M-dwarf multiples have estimated orbital periods less than 50 yr. We have conducted a radial velocity survey of a sample of 29 such targets to complement the astrometric data. This will allow enhanced orbital determinations and precise dynamical masses to be derived in a shorter timeframe than possible with astrometric monitoring alone, and allow for a more reliable isochronal analysis. Here we present radial velocity measurements derived for our sample over several epochs. We report the detection of the three-component spectroscopic multiple 2MASS J05301858-5358483, for which the C component is a new discovery, and forms a tight pair with the B component. Originally identified as a YMG member, we find that this system is a likely old field interloper, whose high chromospheric activity level is caused by tidal spin-up of the tight BC pair. Two other triple systems with a tight pair exist in the sample, 2MASS J04244260-0647313 (previously known) and 2MASS J20163382-0711456, but for the rest of the targets we find that additional tidally synchronized companions are highly unlikely, providing further evidence that their high chromospheric activity levels are generally signatures of youth.
机译:低质量双星的识别和表征对于一系列的天体物理学研究非常重要。太阳附近的年轻(〜10-100 Myr)运动群(YMGs)中的低质量二进制具有特别的意义,因为它们提供了独特的机会来校准恒星模型并评估这些群本身的年龄和年代。低质量M-矮星的主序列寿命约为〜100 Myr,因此在整个YMG阶段都沿质量-光度轨道不断发展,如果与模型无关的动力学问题,则为精确等时测年提供了理想的实验室。质量可以测量。 AstraLux幸运成像多重性调查最近发现了数百个新的YMG低质量双星,其中M矮倍数的子样本估计了不到50年的轨道周期。我们已经对29个此类目标的样本进行了径向速度调查,以补充天文数据。与仅使用天文监测相比,这将允许在更短的时间范围内获得增强的轨道确定能力和精确的动态质量,并允许更可靠的等时线分析。在这里,我们介绍了在几个时期内为我们的样本导出的径向速度测量值。我们报告了对三组分光谱多重2MASS J05301858-5358483的检测,其中C组分是一个新发现,并与B组分形成了紧密的对。最初被确定为YMG成员,我们发现该系统很可能是老场闯入者,其高色球活动水平是由紧密BC对的潮汐旋转引起的。样本中还存在另外两个具有紧密对的三元系统,即2MASS J04244260-0647313(先前已知)和2MASS J20163382-0711456,但对于其余目标,我们发现额外的潮汐同步伴星极不可能,这提供了进一步的证据表明较高的色球活动水平通常是青年的特征。

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