Revealing the inner circumstellar disk of the T Tauri star S Coronae Australis N using the VLTI - Archive ouverte HAL Access content directly
Journal Articles Astronomy and Astrophysics - A&A Year : 2012

Revealing the inner circumstellar disk of the T Tauri star S Coronae Australis N using the VLTI

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J. Vural
  • Function : Author
A. Kreplin
  • Function : Author
S. Kraus
  • Function : Author
G. Weigelt
T. Driebe
  • Function : Author
M. Benisty
M. Dugué
  • Function : Author
F. Massi
  • Function : Author
M. Vannier
  • Function : Author

Abstract


Aims: We investigate the structure of the circumstellar disk of the T Tauri star S CrA N and test whether the observations agree with the standard picture proposed for Herbig Ae stars.
Methods: Our observations were carried out with the VLTI/AMBER instrument in the H and K bands with the low spectral resolution mode. For the interpretation of our near-infrared AMBER and archival mid-infrared MIDI visibilities, we employed both geometric and temperature-gradient models.
Results: To characterize the disk size, we first fitted geometric models consisting of a stellar point source, a ring-shaped disk, and a halo structure to the visibilities. In the H and K bands, we measured ring-fit radii of 0.73 ± 0.03 mas (corresponding to 0.095 ± 0.018 AU for a distance of 130 pc) and 0.85 ± 0.07 mas (0.111 ± 0.026 AU), respectively. This K-band radius is approximately two times larger than the dust sublimation radius of ≈0.05 AU expected for a dust sublimation temperature of 1500 K and gray dust opacities, but approximately agrees with the prediction of models including backwarming (namely a radius of ≈0.12 AU). The derived temperature-gradient models suggest that the disk is approximately face-on consisting of two disk components with a gap between star and disk. The inner disk component has a temperature close to the dust sublimation temperature and a quite narrow intensity distribution with a radial extension from 0.11 AU to 0.14 AU.
Conclusions: Both our geometric and temperature-gradient models suggest that the T Tauri star S CrA N is surrounded by a circumstellar disk that is truncated at an inner radius of ≈ 0.11 AU. The narrow extension of the inner temperature-gradient disk component implies that there is a hot inner rim.

Based on observations made with ESO telescopes at the La Silla Paranal Observatory under program IDs 081.C-0272(A), 083.C-0236(C).

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insu-03612420 , version 1 (18-03-2022)

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Attribution - CC BY 4.0

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J. Vural, A. Kreplin, S. Kraus, G. Weigelt, T. Driebe, et al.. Revealing the inner circumstellar disk of the T Tauri star S Coronae Australis N using the VLTI. Astronomy and Astrophysics - A&A, 2012, 543, ⟨10.1051/0004-6361/201218892⟩. ⟨insu-03612420⟩
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