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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



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ID: 421695.0, MPI für Astronomie / Publikationen_mpia
Cavities in inner disks: the GM Aurigae case
Authors:Dutrey, A.; Guilloteau, S.; Piétu, V.; Chapillon, E.; Gueth, F.; Henning, T.; Launhardt, R.; Pavlyuchenkov, Y.; Schreyer, K.; Semenov, D.
Language:English
Date of Publication (YYYY-MM-DD):2008
Title of Journal:Astronomy and Astrophysics
Volume:490
Start Page:L15
End Page:L18
Review Status:Peer-review
Audience:Experts Only
Abstract / Description:Context: Recent modeling based on unresolved infrared observations of the spectral energy distribution (SED) of GM Aurigae suggests that the inner disk of this single TTauri star is truncated at an inner radius of 25 AU. Aims: We attempt to find evidence of this inner hole in the gas distribution, using spectroscopy with high angular resolution. Methods: Using the IRAM array, we obtained high angular resolution ( 1.5'') observations with a high S/N per channel of the 13CO J=2{-}1 and C18O J=2{-}1 and of the 13CO J=1{-}0 lines. A standard parametric disk model is used to fit the line data in the Fourier-plane and to derive the CO disk properties. Our measurement is based on a detailed analysis of the spectroscopic profile from the CO disk rotating in Keplerian velocity. The millimeter continuum, tracing the dust, is also analyzed. Results: We detect an inner cavity of radius 19 ± 4 AU at the 4.5sigma level. The hole manifests itself by a lack of emission beyond the (projected) Keplerian speed at the inner radius. We also constrain the temperature gradient in the disk. Conclusions: Our data reveal the existence of an inner hole in GM Aur gas disk. Its origin remains unclear, but can be linked to planet formation or to a low mass stellar companion orbiting close to the central star ( 5-15 AU). The frequent finding of inner cavities suggests that either binarity is the most common scenario of star formation in Taurus or that giant planet formation starts early. Based on observations carried out with the IRAM Plateau de Bure Interferometer. IRAM is supported by INSU/CNRS (France), MPG (Germany) and IGN (Spain).
Free Keywords:stars: formation; ISM: molecules; stars: circumstellar matter; radio lines: stars; stars: individual: GM Aurigae
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2008A%26A...490L..15... [ID No:1]
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