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首页> 外文期刊>PASJ: Publications of the Astronomical Society of Japan >Extreme asymmetry in the polarized disk of V1247??Orionis
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Extreme asymmetry in the polarized disk of V1247??Orionis

机译:V1247 Orionis的偏振片中的极端不对称

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Wepresentthefirstnear-infraredscattered-lightdetectionofthetransitionaldiskaroundV1247a€‰Ori,whichwasobtainedusinghigh-resolutionpolarimetricdifferentialimagingobservationswithSubaru/HiCIAO.OurimagingintheHbandrevealsthediskmorphologyatseparationsofa??0$${^{primeprime}_{.}}$$14a€“0$${^{primeprime}_{.}}$$86(54a€“330a€‰au)fromthecentralstar.Thepolarizedintensityimageshowsaremarkablearc-likestructuretowardthesoutheastofthestar,whereasthefainternorthwestregiondoesnotexhibitanynotablefeatures.Theshapeofthearmisconsistentwithanarcof0$${^{primeprime}_{.}}$$28?±0$${^{primeprime}_{.}}$$09inradius(108a€‰aufromthestar),althoughthepossibilityofaspiralarmwithasmallpitchanglecannotbeexcluded.V1247a€‰Orifeaturesanexceptionallylargeazimuthalcontrastinscattered,polarizedlight;theradialpeakofthesoutheasternarcisaboutthreetimesbrighterthanthenorthwesterndiskmeasuredatthesamedistancefromthestar.Combinedwiththepreviousindicationofaninhomogeneousdensitydistributioninthegapata‰246a€‰au,thenotableasymmetryintheouterdisksuggeststhepresenceofunseencompanionsand/orplanet-formingprocessesongoinginthearc.
机译:我们对Ori周围的过渡磁盘进行了首次近红外散射光检测,该光是通过Subaru / HiCIAO的高分辨率偏振差分成像观测获得的。我们在Hband上显示了0a $$ {^ $ {{} $} {}}分离的磁盘形态。来自中央星的$ 86(54a“ 330a au”)。极化强度图像显示出朝着星的另一端很明显的类似弧的结构,而西北偏远地区则有明显的特征。手臂的形状与anarcof0 $$$$ {$$$$$} {{} {{primeprime}} _ {{}}一致。 V1247a的特征是,除非有一个大螺距的星际辐射,否则它的偏振光是散布的,偏振光不大;在不考虑其偏差的情况下,该星状星团的辐射力在同一方向上一直保持着一个均匀的方向,直到它与之保持一致。外部磁盘建议在电弧中持续存在看不见的伴侣和/或行星形成过程。

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