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HD 139614: the interferometric case for a group-Ib pre-transitional young disk

机译:HD 139614:Ib组过渡前年轻磁盘的干涉仪案例

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The Herbig Ae star HD 139614 is a group-Ib object, which featureless SED indicates disk flaring and a possible pre-transitional evolutionary stage. We present mid- and near-IR interferometric results collected with MIDI, AMBER and PIONIER with the aim of constraining the spatial structure of the 0.1-10 AU disk region and assess its possible multi-component structure. A two-component disk model composed of an optically thin 2-AU wide inner disk and an outer temperature-gradient disk starting at 5.6 AU reproduces well the observations. This is an additional argument to the idea that group-Ⅰ HAeBe inner disks could be already in the disk-clearing transient stage. HD 139614 will become a prime target for mid-IR interferometric imaging with the second-generation instrument MATISSE of the VLTI.
机译:Herbig Ae星HD 139614是一个Ib组物体,其无特征的SED指示盘张开,并可能有过渡前的演化阶段。我们介绍了用MIDI,AMBER和PIONIER收集的中红外和近红外干涉测量结果,目的是限制0.1-10 AU磁盘区域的空间结构,并评估其可能的多分量结构。由光学上较薄的2-AU宽的内部磁盘和从5.6 AU开始的外部温度梯度磁盘组成的两成分磁盘模型可以很好地再现观察结果。这是Ⅰ组HAeBe内部磁盘可能已经处于清除磁盘过渡阶段的想法的另一个论点。 HD 139614将通过VLTI的第二代仪器MATISSE成为中红外干涉成像的主要目标。

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