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Planet-disk interactions in HD 169142? Tracing ellipticity, structures, and offsets

机译:HD 169142中的行星磁盘交互? 跟踪椭圆形,结构和偏移

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In Bertrang et al. (2018), we present new data of the protoplanetary disk surrounding the Herbig Ae/Be star HD 169142 obtained in the very broad-band (VBB) with the Zurich imaging polarimeter (ZIMPOL), a subsystem of the Spectro-Polarimetric High-contrast Exoplanet REsearch instrument (SPHERE) at the Very Large Telescope (VLT). Our Polarimetric Differential Imaging (PDI) observations probe the disk as close as 0.″03 (3.5 au) to the star and are able to trace the disk out to ~1.″08(~ 126 au). We find an inner hole, a bright ring bearing substructures around 0.″18 (21 au), and an elliptically shaped gap stretching from 0.″25 to 0.″47 (29 - 55 au). Outside of 0.″47, the surface brightness drops off, discontinued only by a narrow annular brightness minimum at ~ 0.″63 - 0.″74 (74 - 87 au). These observations confirm features found in less-well resolved data as well as reveal yet undetected indications for planet-disk interactions, such as small-scale structures, star-disk offsets, and potentially moving shadows.
机译:在Bertrang等。 (2018),我们呈现出在非常宽带(VBB)中获得的Herbig AE / BES星HD 169142的原始圆盘的新数据与苏黎希成像偏振仪(ZIMPOL),Spectro-Polariemetric高对比度的子系统在非常大的望远镜(VLT)的Exoplanet研究仪器(球体)。我们的Polariemetric差分成像(PDI)观察探测磁盘尽可能接近0.“03(3.5 AU),并且能够将磁盘追踪到〜1。”08(〜126 AU)。我们发现一个内孔,亮环轴承轴围绕0.“18(21Au),椭圆形间隙从0.”25至0.“47(29-55AU)。在0.“47中,表面亮度下降,仅在〜0”63-0“的窄环形亮度最小停留。74(74-87AU)。这些观察结果确认了在不太好的解决数据中发现的功能,并揭示了行星磁盘交互的尚未检测到的指示,例如小规模结构,星形偏移和可能移动的阴影。

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