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Substructure in the Circumstellar Disk Around the Young Star AU Microscopii

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Liu, Michael C.·2004·Science

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 β 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 ≈12 million years.

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Metadata

Authors
Liu, M. C.
Venue
Science
Published
2004-09-03
Volume
305
Issue
5689
Pages
1442-1444
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2022546175
Cited by
165
References
0
FWCI
8.47
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Substructure in the Circumstellar Disk Around the Young Star AU Microscopii. https://app.cochat.ai/papers/10.1126/science.1102929
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Liu, M. C. (2004). Substructure in the Circumstellar Disk Around the Young Star AU Microscopii. Science. https://doi.org/10.1126/science.1102929

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