High-resolution thermal infrared imaging of MWC300. VLT/VISIR observations in BURST mode
Résumé
Context: B[e] stars are expected to possess dusty circumstellar environments, which are responsible for a strong infrared (IR) excess.
Aims: Using single-dish diffraction-limited imaging in the thermal infrared domain, we aim at measuring the angular extension of the dusty environment of the galactic B[e] MWC 300.
Methods: We obtained diffraction-limited images of MWC 300 at 11.25 mum using the BURST mode of the VLT/VISIR instrument.
Results: MWC 300 is partially, but statistically significantly, resolved by VISIR so that we could measure the size of its dusty envelope for the first time. By assuming a 2D circular Gaussian intensity distribution and using different image analysis methods we measured a FWHM angular size of 69 ± 10 mas. For a distance of 1.8 kpc, we obtain a linear size of 125±18 AU = (1.87±0.26) × 1013 m for the circumstellar dust emitting in the mid-IR. This measured size is shown to agree with a model that was calculated with our radiative radiative transfer code and constrained by previously reported SED data. Additionally, the flux of MWC 300 at 11.25 mum is estimated as 84.5±1.4 Jy = (20.0±0.3) × 10-13 W/m^2/mum.
Conclusions: The VLT/VISIR now offers the possibility of obtaining mid-IR diffraction-limited images with a high signal-to-noise ratio. The MWC 300's size as directly measured in this work is compatible with the theoretical size of a nearly edge-on dusty disc estimated in previous works. Interferometric data at milliarcsec angular resolution are required to reveal details on this dusty envelope.
Aims: Using single-dish diffraction-limited imaging in the thermal infrared domain, we aim at measuring the angular extension of the dusty environment of the galactic B[e] MWC 300.
Methods: We obtained diffraction-limited images of MWC 300 at 11.25 mum using the BURST mode of the VLT/VISIR instrument.
Results: MWC 300 is partially, but statistically significantly, resolved by VISIR so that we could measure the size of its dusty envelope for the first time. By assuming a 2D circular Gaussian intensity distribution and using different image analysis methods we measured a FWHM angular size of 69 ± 10 mas. For a distance of 1.8 kpc, we obtain a linear size of 125±18 AU = (1.87±0.26) × 1013 m for the circumstellar dust emitting in the mid-IR. This measured size is shown to agree with a model that was calculated with our radiative radiative transfer code and constrained by previously reported SED data. Additionally, the flux of MWC 300 at 11.25 mum is estimated as 84.5±1.4 Jy = (20.0±0.3) × 10-13 W/m^2/mum.
Conclusions: The VLT/VISIR now offers the possibility of obtaining mid-IR diffraction-limited images with a high signal-to-noise ratio. The MWC 300's size as directly measured in this work is compatible with the theoretical size of a nearly edge-on dusty disc estimated in previous works. Interferometric data at milliarcsec angular resolution are required to reveal details on this dusty envelope.
Domaines
Astrophysique [astro-ph]
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