Herschel images of Fomalhaut An extrasolar Kuiper belt at the height of its dynamical activity
Artikel i vetenskaplig tidskrift, 2012
Context. Fomalhaut is a young (2 +/- 1 x 10(8) years), nearby (7.7 pc), 2 M-circle dot star that is suspected to harbor an infant planetary system, interspersed with one or more belts of dusty debris. Aims. We present far-infrared images obtained with the Herschel Space Observatory with an angular resolution between 5.7 '' and 36.7 '' at wavelengths between 70 mu m and 500 mu m. The images show the main debris belt in great detail. Even at high spatial resolution, the belt appears smooth. The region in between the belt and the central star is not devoid of material; thermal emission is observed here as well. Also at the location of the star, excess emission is detected. We aim to construct a consistent image of the Fomalhaut system. Methods. We use a dynamical model together with radiative-transfer tools to derive the parameters of the debris disk. We include detailed models of the interaction of the dust grains with radiation, for both the radiation pressure and the temperature determination. Comparing these models to the spatially resolved temperature information contained in the images allows us to place strong constraints on the presence of grains that will be blown out of the system by radiation pressure. We use this to derive the dynamical parameters of the system. Results. The appearance of the belt points toward a remarkably active system in which dust grains are produced at a very high rate by a collisional cascade in a narrow region filled with dynamically excited planetesimals. Dust particles with sizes below the blow-out size are abundantly present. The equivalent of 2000 one-km-sized comets are destroyed every day, out of a cometary reservoir amounting to 110 Earth masses. From comparison of their scattering and thermal properties, we find evidence that the dust grains are fluffy aggregates, which indicates a cometary origin. The excess emission at the location of the star may be produced by hot dust with a range of temperatures, but may also be due to gaseous free-free emission from a stellar wind.
light
evolution
stars: individual: Fomalhaut
stars
grains
planetary systems
circumstellar matter
spire instrument
dust
small particles
radiation
debris disk
planetary system
Författare
B. Acke
KU Leuven
M. Min
Universiteit Utrecht
Anton Pannekoek Institute for Astronomy
C. Dominik
Radboud Universiteit
Anton Pannekoek Institute for Astronomy
B. Vandenbussche
KU Leuven
B. Sibthorpe
Royal Observatory
C. Waelkens
KU Leuven
G. Olofsson
Stockholms universitet
P. Degroote
KU Leuven
K. Smolders
KU Leuven
E. Pantin
Centre national de la recherche scientifique (CNRS)
M. J. Barlow
University College London (UCL)
Jadl Blommaert
KU Leuven
A. Brandeker
Stockholms universitet
W. De Meester
KU Leuven
W. R. F. Dent
Atacama Large Millimeter-submillimeter Array (ALMA)
K. M. Exter
KU Leuven
J. Di Francesco
National Research Council Canada
M. Fridlund
Europeiska rymdorganisationen (ESA)
W. K. Gear
Cardiff University
A. M. Glauser
Eidgenössische Technische Hochschule Zürich (ETH)
Royal Observatory
J. S. Greaves
University of St Andrews
P. M. Harvey
The University of Texas at Austin
T. Henning
Max-Planck-Gesellschaft
M. R. Hogerheijde
Universiteit Leiden
W. S. Holland
Royal Observatory
R. Huygen
KU Leuven
R. J. Ivison
University of Edinburgh
Royal Observatory
C. Jean
KU Leuven
René Liseau
Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik
D. A. Naylor
University of Lethbridge
G.L. Pilbratt
Europeiska rymdorganisationen (ESA)
E. T. Polehampton
STFC Rutherford Appleton Laboratory
University of Lethbridge
S. Regibo
KU Leuven
P. Royer
KU Leuven
A. Sicilia-Aguilar
Max-Planck-Gesellschaft
Universidad Autonoma de Madrid (UAM)
B. M. Swinyard
STFC Rutherford Appleton Laboratory
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 540 Article Number: A125 - A125Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
DOI
10.1051/0004-6361/201118581