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          Institute: MPI für Astrophysik     Collection: High Energy Astrophysics at MPA     Display Documents

ID: 14628.0, MPI für Astrophysik / High Energy Astrophysics at MPA
The dust disk of HR 4049 - Another brick in the wall
Authors:Dominik, C.; Dullemond, C. P.; Cami, J.; van Winckel, H.
Date of Publication (YYYY-MM-DD):2003-01
Title of Journal:Astronomy & Astrophysics
Journal Abbrev.:Astron. Astrophys.
Issue / Number:2
Start Page:595
End Page:609
Review Status:Peer-review
Audience:Experts Only
Abstract / Description:We present the Spectral Energy Distribution of HR 4049 based on literature data and new continuum measurements at 850 mum. The SED shows variable absorption in the UV, and a large IR excess, both caused by circumstellar dust. The shape of the IR excess from 1 mum all the way down to 850 mum can be nearly perfectly fitted with a single blackbody function at T approximate to1150 K or alternatively with a sum of blackbodies in a narrow temperature range. The energy emitted in this IR continuum radiation is about one-third of the stellar luminosity. We show that this blackbody radiation must be due to the presence of a circumbinary disk with a large height. This disk must also be gas-rich, in agreement with the observations of molecular bands in the ISO-SWS spectrum. We present two possible scenario's for explaining the shape and the intensity of the IR excess. The first scenario involves large grains (a greater than or equal to 1 mm) that each radiate like a blackbody. The second scenario argues that the blackbody radiation is due to a very optically thick circumbinary disk. We investigate if such a disk would indeed produce blackbody radiation by presenting results from radiative transfer calculations. We further quantify the properties of such a disk and its stability in the framework of (hydro)dynamics, grain settling, radiation pressure and grain drift. The virtues and shortcomings of both models for the origin of the IR blackbody are discussed by contrasting them with other observations and assessing them in the framework of (binary) (post-)AGB evolution.
Free Keywords:circumstellar matter; infrared : stars; binaries : spectroscopic; stars : evolution; stars : variables : general
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astrophysik
External Affiliations:Sterrekundig Inst Anton Pannekoek, Kruislaan 403, NL-1098 SJ; Amsterdam, Netherlands; Sterrekundig Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands; Max Planck Inst Astrophys, D-85748 Garching, Germany; SRON Groningen, NL-9700 AV Groningen, Netherlands; Katholieke Univ Leuven, Sterrekundig Inst, B-3001 Heverlee, Belgium
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