The AU Mic Debris Disk: Far-Infrared and Submillimeter Resolved Imaging
Artikel i vetenskaplig tidskrift, 2015

We present far-infrared and submillimeter maps from the Herschel Space Observatory and the James Clerk Maxwell Telescope of the debris disk host star AU Microscopii. Disk emission is detected at 70, 160, 250, 350, 450, 500, and 850 μm. The disk is resolved at 70, 160, and 450 μm. In addition to the planetesimal belt, we detect thermal emission from AU Mic's halo for the first time. In contrast to the scattered light images, no asymmetries are evident in the disk. The fractional luminosity of the disk is and its milimeter-grain dust mass is (±20%). We create a simple spatial model that reconciles the disk spectral energy distribution as a blackbody of 53 ± 2 K (a composite of 39 and 50 K components) and the presence of small (non-blackbody) grains which populate the extended halo. The best-fit model is consistent with the "birth ring" model explored in earlier works, i.e., an edge-on dust belt extending from 8.8 to 40 AU, but with an additional halo component with an surface density profile extending to the limits of sensitivity (140 AU). We confirm that AU Mic does not exert enough radiation force to blow out grains. For stellar mass-loss rates of 10-100 times solar, compact (zero porosity) grains can only be removed if they are very small; consistently with previous work, if the porosity is 0.9, then grains approaching 0.1 μm can be removed via corpuscular forces (i.e., the stellar wind).

stars: individual (AU Mic)

circumstellar matter


B. C. Matthews

National Research Council Canada

University of Victoria

G. Kennedy

University of Cambridge

B. Sibthorpe

Netherlands Institute for Space Research (SRON)

W. S. Holland

Royal Observatory

University of Edinburgh

M. Booth

Pontificia Universidad Catolica de Chile

P. Kalas

University of California

SETI Institute

M. Macgregor

Harvard-Smithsonian Center for Astrophysics

D. J. Wilner

Harvard-Smithsonian Center for Astrophysics

B. Vandenbussche

KU Leuven

G. Olofsson

AlbaNova University Center

Jadl Blommaert

Vlaamse Instelling voor Technologisch Onderzoek (VITO)

Vrije Universiteit Brüssel (VUB)

A. Brandeker

AlbaNova University Center

W. R. F. Dent

Atacama Large Millimeter-submillimeter Array (ALMA)

B. L. D. Vries

Stockholms universitet

AlbaNova University Center

J. D. Francesco

University of Victoria

National Research Council Canada

Malcolm Fridlund

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

J. R. Graham

University of California

J. S. Greaves

University of St Andrews

A. Heras

European Space Research and Technology Centre (ESA ESTEC)

M. Hogerheijde

Universiteit Leiden

R. J. Ivison

University of Edinburgh

European Southern Observatory (ESO)

E. Pantin

Centre national de la recherche scientifique (CNRS)

G.L. Pilbratt

European Space Research and Technology Centre (ESA ESTEC)

Astrophysical Journal

0004-637X (ISSN) 1538-4357 (eISSN)

Vol. 811 2 100- 100


Astronomi, astrofysik och kosmologi



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