2018A&A...616A.153K


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.13CEST07:40:48

2018A&A...616A.153K - Astronomy and Astrophysics, volume 616A, 153-153 (2018/8-1)

The perturbed sublimation rim of the dust disk around the post-AGB binary IRAS08544-4431.

KLUSKA J., HILLEN M., VAN WINCKEL H., MANICK R., MIN M., REGIBO S. and ROYER P.

Abstract (from CDS):


Context. Post-asymptotic giant branch (post-AGB) binaries are surrounded by stable dusty and gaseous disks similar to the ones around young stellar objects. Whereas, significant effort has been spent on modeling observations of disks around young stellar objects, the disks around post-AGB binaries have received significantly less attention, even though they pose significant constraints on theories of disk physics and binary evolution.
Aims. We want to examine the structure of and phenomena at play in circumbinary disks around post-AGB stars. We continue the analysis of our near-infrared interferometric image of the inner rim of the circumbinary disk around IRAS08544-4431. We want to understand the physics governing this inner disk rim.
Methods. We use a radiative transfer model of a dusty disk to reproduce simultaneously the photometry as well as the near-infrared interferometric dataset on IRAS08544-4431. The model assumes hydrostatic equilibrium and takes dust settling self-consistently into account.
Results. The best-fit radiative transfer model shows excellent agreement with the spectral energy distribution up to millimeter wavelengths as well as with the PIONIER visibility data. It requires a rounded inner rim structure, starting at a radius of 8.25 au. However, the model does not fully reproduce the detected over-resolved flux nor the azimuthal flux distribution of the inner rim. While the asymmetric inner disk rim structure is likely to be the consequence of disk-binary interactions, the origin of the additional over-resolved flux remains unclear.
Conclusions. As in young stellar objects, the disk inner rim of IRAS08544-4431 is ruled by dust sublimation physics. Additional observations are needed to understand the origin of the extended flux and the azimuthal perturbation at the inner rim of the disk.

Abstract Copyright: © ESO 2018

Journal keyword(s): stars: AGB and post-AGB - binaries: general - circumstellar matter - stars: individual: IRAS 08544-4431 - radiative transfer

Simbad objects: 3

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Number of rows : 3

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 5669 1
2 CD-44 4961 pA* 08 56 14.1790943091 -44 43 10.710041643   10.55 9.176     F3e 57 1
3 * 89 Her pA* 17 55 25.1884459710 +26 02 59.970100296 5.36 5.70 5.36 5.06 4.94 F2Ibp 386 0

    Equat.    Gal    SGal    Ecl

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2020.07.13-07:40:48

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