A multi-wavelength interferometric study of the massive young stellar object IRAS 13481-6124
arXiv:1511.03195 · doi:10.1051/0004-6361/201527502
Abstract
We present new mid-infrared interferometric observations of the massive young stellar object IRAS 13481-6124, using VLTI/MIDI for spectrally-resolved, long-baseline measurements (projected baselines up to m) and GSO/T-ReCS for aperture-masking interferometry in five narrow-band filters (projected baselines of m) in the wavelength range of m. We combine these measurements with previously-published interferometric observations in the and bands in order to assemble the largest collection of infrared interferometric observations for a massive YSO to date. Using a combination of geometric and radiative-transfer models, we confirm the detection at mid-infrared wavelengths of the disk previously inferred from near-infrared observations. We show that the outflow cavity is also detected at both near- and mid-infrared wavelengths, and in fact dominates the mid-infrared emission in terms of total flux. For the disk, we derive the inner radius ( mas or AU at 3.6 kpc), temperature at the inner rim ( K), inclination ( deg) and position angle ( deg). We determine that the mass of the disk cannot be constrained without high-resolution observations in the (sub-)millimeter regime or observations of the disk kinematics, and could be anywhere from to M. Finally, we discuss the prospects of interpreting the spectral energy distributions of deeply-embedded massive YSOs, and warn against attempting to infer disk properties from the SED.
Accepted to Astronomy and Astrophysics
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