论文标题

可能的二进制protostar Z CMA的飞越。

A likely flyby of binary protostar Z CMa caught in action

论文作者

Dong, Ruobing, Liu, Hauyu Baobab, Cuello, Nicolas, Pinte, Christophe, Abraham, Peter, Vorobyov, Eduard, Hashimoto, Jun, Kospal, Agnes, Chiang, Eugene, Takami, Michihiro, Chen, Lei, Dunham, Michael, Fukagawa, Misato, Green, Joel, Hasegawa, Yasuhiro, Henning, Thomas, Pavlyuchenkov, Yaroslav, Pyo, Tae-Soo, Tamura, Motohide

论文摘要

在恒星形成簇中,年轻的恒星物体之间的紧密相遇预计将极大地扰动情节磁盘。这些事件在恒星形成的数值模拟中见证了,但很少有对正在进行的遭遇的直接观察。在这里,我们报告了Sub-0” .1分辨率Atacama大毫米阵列(Alma)和Jansky非常大的阵列(JVLA)观察到对百万年历史的二元二元protostar Z CMA中的尘埃和分子线排放。散落的光成像,其在灰尘和气体发射方面的对应物也与模拟相比,表明在行动中罕见的飞行事件的路标是“双重毛bur”。

Close encounters between young stellar objects in star forming clusters are expected to dramatically perturb circumstellar disks. Such events are witnessed in numerical simulations of star formation, but few direct observations of ongoing encounters have been made. Here we report sub-0".1 resolution Atacama Large Millimeter Array (ALMA) and Jansky Very Large Array (JVLA) observations towards the million year old binary protostar Z CMa in dust continuum and molecular line emission. A point source ~4700 au from the binary has been discovered at both millimeter and centimeter wavelengths. It is located along the extension of a ~2000 au streamer structure previously found in scattered light imaging, whose counterpart in dust and gas emission is also newly identified. Comparison with simulations shows signposts of a rare flyby event in action. Z CMa is a "double burster", as both binary components undergo accretion outbursts, which may be facilitated by perturbations to the host disk by flybys.

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