Fast-moving features in the debris disk around AU Microscopii

Meyer Michael R.; Moutou Claire; Olofsson Johan; Rodigas Timothy; Sauvage Jean-Francois; Schlieder Joshua; Schmid Hans Martin; Turatto Massimo; Udry Stephane; Vakili Farrokh; Boccaletti Anthony; Thalmann Christian; Vigan Arthur; Wahhaj Zahed; Lagrange Anne-Marie; Janson Markus; Augereau Jean-Charles; Schneider Glenn; Milli Julien; Grady Carol; Debes John; Langlois Maud; Mouillet David; Henning Thomas; Dominik Carsten; Maire Anne-Lise; Beuzit Jean-Luc; Carson Joseph; Dohlen Kjetil; Engler Natalia; Feldt Markus; Fusco Thierry; Ginski Christian; Girard Julien H.; Hines Dean; Kasper Markus; Mawet Dimitri; Menard Franois; Wisniewski John

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Fast-moving features in the debris disk around AU Microscopii

机译：AU Microscopii周围的碎片磁盘中的快速移动功能

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In the 1980s, excess infrared emission was discovered around main-sequence stars; subsequent direct-imaging observations revealed orbiting disks of cold dust to be the source(1). These 'debris disks' were thought to be by-products of planet formation because they often exhibited morphological and brightness asymmetries that may result from gravitational perturbation by planets. This was proved to be true for the beta Pictoris system, in which the known planet generates an observable warp in the

机译：在1980年代，在主要序列恒星周围发现了过量的红外辐射。随后的直接成像观测表明，冷尘盘绕轨道是源（1）。这些“碎片盘”被认为是行星形成的副产品，因为它们经常表现出形态和亮度的不对称性，这可能是由于行星的引力扰动引起的。事实证明，这对于Beta Pictoris系统是正确的，在该系统中，已知行星在行星中产生了可观察到的扭曲。

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来源
《Nature》 |2015年第7572期|230-232|共3页
作者
Meyer Michael R.; Moutou Claire; Olofsson Johan; Rodigas Timothy; Sauvage Jean-Francois; Schlieder Joshua; Schmid Hans Martin; Turatto Massimo; Udry Stephane; Vakili Farrokh; Boccaletti Anthony; Thalmann Christian; Vigan Arthur; Wahhaj Zahed; Lagrange Anne-Marie; Janson Markus; Augereau Jean-Charles; Schneider Glenn; Milli Julien; Grady Carol; Debes John; Langlois Maud; Mouillet David; Henning Thomas; Dominik Carsten; Maire Anne-Lise; Beuzit Jean-Luc; Carson Joseph; Dohlen Kjetil; Engler Natalia; Feldt Markus; Fusco Thierry; Ginski Christian; Girard Julien H.; Hines Dean; Kasper Markus; Mawet Dimitri; Menard Franois; Wisniewski John;
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作者单位

ETH, Inst Astron, CH-8093 Zurich, Switzerland.;

Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.;

Max Planck Inst Astron, D-69117 Heidelberg, Germany.;

Carnegie Inst Sci, Dept Terr Magnetism, Washington, DC 20015 USA.;

Off Natl Etud & Rech Aerosp, F-92322 Chatillon, France.;

NASA, Ames Res Ctr, Space Sci & Astrobiol Div, Moffett Field, CA 94035 USA.;

ETH, Inst Astron, CH-8093 Zurich, Switzerland.;

INAF Osservatorio Astron Padova, I-35122 Padua, Italy.;

Univ Geneva, Observ Geneve, CH-1290 Versoix, Switzerland.;

Univ Nice Sophia Antipolis UNS, CNRS, Lab JL Lagrange, OCA, F-06108 Nice 2, France.;

Univ Paris 06, Univ Paris Diderot, CNRS, Observ Paris,LESIA, F-92190 Meudon, France.;

ETH, Inst Astron, CH-8093 Zurich, Switzerland.;

Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.;

Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.;

IPAG, CNRS, F-38000 Grenoble, France.;

Max Planck Inst Astron, D-69117 Heidelberg, Germany.;

IPAG, CNRS, F-38000 Grenoble, France.;

Univ Arizona, Steward Observ, Tucson, AZ 85721 USA.;

ESO, Santiago 19001, Chile.;

Eureka Sci, Oakland, CA 96002 USA.;

Space Telescope Sci Inst, Baltimore, MD 21218 USA.;

Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.;

Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France.;

Max Planck Inst Astron, D-69117 Heidelberg, Germany.;

Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 XH Amsterdam, Netherlands.;

INAF Osservatorio Astron Padova, I-35122 Padua, Italy.;

IPAG, CNRS, F-38000 Grenoble, France.;

Coll Charleston, Dept Phys & Astron, Charleston, SC 29424 USA.;

Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.;

ETH, Inst Astron, CH-8093 Zurich, Switzerland.;

Off Natl Etud & Rech Aerosp, F-92322 Chatillon, France.;

Sterrewacht Leiden, NL-2300 RA Leiden, Netherlands.;

ESO, Santiago 19001, Chile.;

Space Telescope Sci Inst, Baltimore, MD 21218 USA.;

ESO, D-85748 Garching, Germany.;

CALTECH, Dept Astron, Pasadena, CA 91125 USA.;

Univ Chile, Dept Astron, Santiago, Chile.;

Univ Oklahoma, Dept Phys & Astron, Norman, OK 73019 USA.;

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入库时间 2022-08-18 02:52:42

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1. Observations of fast-moving features in the debris disk of AU Mic on a three-year timescale: Confirmation and new discoveries ★ ★★ [J] . A. Boccaletti, E. Sezestre, A.-M. Lagrange, Astronomy and astrophysics . 2018,第19期

机译：在三年时间内观察到的AU Mic碎片盘中快速移动的特征：确认和新发现★ ★★
2. DUST DYNAMICS, SURFACE BRIGHTNESS PROFILES, AND THERMAL SPECTRA OF DEBRIS DISKS: THE CASE OF AU MICROSCOPII [J] . LINDA E. STRUBBE, EUGENE I. CHIANG The Astrophysical journal . 2006,第1Pt1期

机译：圆盘的粉尘动力学，表面亮度分布和热光谱：以金相显微镜为例
3. DUST DYNAMICS, SURFACE BRIGHTNESS PROFILES, AND THERMAL SPECTRA OF DEBRIS DISKS: THE CASE OF AU MICROSCOPII [J] . LINDA E. STRUBBE, EUGENE I. CHIANG The Astrophysical journal . 2006,第1Pt1期

机译：尘埃动力学，表面亮度分布和碎片盘的热谱：以金相显微镜为例
4. A Resolved Millimeter Emission Belt in the AU Mic Debris Disk [C] . Meredith MacGregor International Astronomical Union. . 2013

机译：Au MIC碎片盘中的分辨毫米排放带
5. Searching the solar neighborhood for protoplanetary debris disks: A survey of Vega-like sources and a discussion of new disk examples [D] . Fisher, Robert Scott. 2000

机译：在太阳附近搜寻原行星碎片盘：对类似Vega的震源的调查以及对新盘实例的讨论
6. Postdiskogram CT Features of Lidocaine-Sensitive and Lidocaine-Insensitive Severely Painful Disks at Provocation Lumbar Diskography [O] . W.S. Bartynski, W.E. Rothfus, M. Kurs-Lasky 2008

机译：Lidocaine敏感和Lidocaine-Insensitivey的Postdiskgume CT功能在挑衅腰椎造影中
7. Fast-moving features in the debris disk around AU Microscopii [O] . Boccaletti, Anthony, Thalmann, Christian, Lagrange, Anne-Marie, 2015

机译：AU Microscopii周围的碎片磁盘中的快速移动功能

Fast-moving features in the debris disk around AU Microscopii

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