论文标题
后院世界发现的极冷的棕色矮人的Spitzer随访:9号公民科学项目
Spitzer Follow-up of Extremely Cold Brown Dwarfs Discovered by the Backyard Worlds: Planet 9 Citizen Science Project
论文作者
论文摘要
我们介绍了由后院世界发现的95个候选者的Spitzer后续成像:Planet 9 Citizen Science Project,该项目在多上观察图像中使用视觉感知的运动来识别先前未知的子宫邻居在太阳上。我们测量了Spitzer [3.6] - [4.5]颜色以使我们的棕色矮人候选物进行色谱,重点是指出样品中最冷和最接近的y矮人。智慧和烈性天文学的结合提供了对我们75发现的横向运动的定量确认。我们的九个运动确认对象具有大于1“/yr的最佳拟合线性运动;我们最快的动作发现是WISEA J155349.96+693355.2(总运动〜2.15英寸/yr),可能的t类型subdwarf。我们还报告了一个新发现的广泛分离(〜400 au)T8与白矮人LSPM J0055+5948(要找到的第四个这样的系统)的伴侣,再加上一个候选人的候选人,是白dwarf lsr j0002+6357的候选伴侣,在5.5'预计的分隔率(If Isportation)。在我们的运动确认目标中,有五种具有与Y型光谱型的spitzer颜色。这五种具有异常红色的spitzer颜色,暗示了Y1或更高版本的类型,从而在此特别有价值的低温状态下增加了少量已知物体样本。我们的矮人候选人开始弥合大量y矮人人口和最冷的棕色矮人之间的差距。
We present Spitzer follow-up imaging of 95 candidate extremely cold brown dwarfs discovered by the Backyard Worlds: Planet 9 citizen science project, which uses visually perceived motion in multi-epoch WISE images to identify previously unrecognized substellar neighbors to the Sun. We measure Spitzer [3.6]-[4.5] color to phototype our brown dwarf candidates, with an emphasis on pinpointing the coldest and closest Y dwarfs within our sample. The combination of WISE and Spitzer astrometry provides quantitative confirmation of the transverse motion of 75 of our discoveries. Nine of our motion-confirmed objects have best-fit linear motions larger than 1"/yr; our fastest-moving discovery is WISEA J155349.96+693355.2 (total motion ~2.15"/yr), a possible T type subdwarf. We also report a newly discovered wide-separation (~400 AU) T8 comoving companion to the white dwarf LSPM J0055+5948 (the fourth such system to be found), plus a candidate late T companion to the white dwarf LSR J0002+6357 at 5.5' projected separation (~8,700 AU if associated). Among our motion-confirmed targets, five have Spitzer colors most consistent with spectral type Y. Four of these five have exceptionally red Spitzer colors suggesting types of Y1 or later, adding considerably to the small sample of known objects in this especially valuable low-temperature regime. Our Y dwarf candidates begin bridging the gap between the bulk of the Y dwarf population and the coldest known brown dwarf.