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年轻恒星 AU Microscopii 周围星周盘中的子结构。

Substructure in the circumstellar disk around the young star AU Microscopii.

作者信息

Liu Michael C

机构信息

Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA.

出版信息

Science. 2004 Sep 3;305(5689):1442-4. doi: 10.1126/science.1102929. Epub 2004 Aug 12.

Abstract

Keck adaptive optics imaging with a physical resolution of 0.4 astronomical units (AU) resolves the inner (15 to 80 AU) disk of AU Microscopii (AU Mic, GJ 803, HD 197481), the nearest known scattered light disk to Earth. The inner disk is asymmetric and possesses a sharp change in structure at 35 AU. The disk also shows spatially localized enhancements and deficits at 25- to 40-AU separations. The overall morphology points to the influence of unseen larger bodies and resembles structures expected from recent planet formation. AU Mic is coeval with the archetypical debris disk system beta Pictoris, and the similarities between their two disks point to synchronous disk evolution. Multiple indications of substructure appear to be common in circumstellar disks at an age of approximately 12 million years.

摘要

凯克自适应光学成像的物理分辨率为0.4天文单位(AU),它解析出了距地球最近的已知散射光盘——显微镜座AU(AU Mic,GJ 803,HD 197481)的内盘(15至80天文单位)。内盘不对称,在35天文单位处结构有明显变化。该盘在25至40天文单位的间距处还呈现出空间局部增强和亏损。整体形态表明存在未被观测到的较大天体的影响,并且类似于近期行星形成所预期的结构。AU Mic与典型的碎片盘系统绘架座β处于同一时代,它们两个盘之间的相似性表明盘的演化是同步的。在大约1200万年的年龄时,子结构的多种迹象似乎在恒星周围盘中很常见。

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