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Dust temperature and density profiles of AGB and post-AGB stars from mid-infrared observations
Eric Lagadec 1, Djamel Mékarnia 1, José Antonio De Freitas Pacheco 2, Catherine Dougados 3
(2004-11-26)

First mid-infrared images of a sample of AGB and post-AGB carbon stars (V Hya, IRC +10216, CIT 6 and Roberts 22) obtained at La Silla Observatory (ESO, Chile) are reported. CIT 6 presents a cometary-like feature clearly seen in the 9.7$\mu$m image, Roberts 22 shows an envelope slightly elongated in the north-east direction while images of V Hya and IRC+10216 are roughly spherically symmetric. Using inversion technique, the dust emissivity was derived from the observed intensity profiles, allowing a determination of the grain temperature and density distributions inside the envelope for these stars. Dust masses and mass-loss rates were estimated for V\,Hya and IRC\,+10216. Our results are comparable to those obtained in previous studies if dust grains have dimensions in the range $\sim$\,0.01\,-\,0.2\,$\mu$m. Color maps suggest the presence of temperature inhomogeneities in the central regions of the dust envelopes. In the case of V Hya, an eccentric hot point, which direction coincides with the jet previously seen in [SII] emission, suggest that we are observing a material ejected in a previous mass-loss event. Bipolar lobes are clearly seen in the color maps of Roberts 22 and IRC +10216.
1:  Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE)
Université de Nice Sophia Antipolis (UNS) – CNRS : UMR6202 – Observatoire de la Cote d'Azur – INSU
2:  Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS)
Université de Nice Sophia Antipolis (UNS) – CNRS : UMR6162 – Observatoire de la Cote d'Azur – INSU
3:  Laboratoire d'Astrophysique de Grenoble (LAOG)
CNRS : UMR5571 – OSUG – INSU – Université Joseph Fourier - Grenoble I
Sciences of the Universe/Astrophysics

Physics/Astrophysics/Cosmology and Extra-Galactic Astrophysics
AGB and post-AGB – circumstellar matter – mass-loss – imaging – Infrared
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