On the massive young stellar object AFGL4176: High-spatial-resolution multi-wavelength observations and modeling
arXiv:1209.3583 · doi:10.1051/0004-6361/201218905
Abstract
Deeply embedded and at distances of several kiloparsecs, massive young stellar objects (MYSOs) present numerous challenges for observation and study. In this work, we present spatially-resolved observations of one MYSO, AFGL 4176, together with survey and literature data, ranging from interferometric observations with VLTI/MIDI in the mid-infrared, to single-dish Herschel measurements in the far-infrared, and sub-millimeter data from APEX. We consider this spatially-resolved, multi-wavelength data set in terms of both radiative transfer and geometric models. We find that the observations are well described by one-dimensional models overall, but there are also substantial deviations from spherical symmetry at scales of tens to hundreds of astronomical units, which are revealed by the mid-infrared interferometric measurements. We use a multiple-component, geometric modeling approach to explain the mid-infrared emission on scales of tens to hundreds of astronomical units, and find the MIDI measurements are well described by a model consisting of a one-dimensional Gaussian halo and an inclined (θ=60 deg) circumstellar disk extending out to several hundred astronomical units along a position angle of 160 deg. Finally, we compare our results both with previous models of this source, and with those of other MYSOs, and discuss the present situation with mid-infrared interferometric observations of massive stars.
15 pages, 14 figures. Accepted to Astronomy and Astrophysics
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Cited by in corpus (7)
- A Keplerian-like disk around the forming O-type star AFGL 4176
- CO bandhead emission of massive young stellar objects: determining disc properties
- The VLTI/MIDI survey of massive young stellar objects - Sounding the inner regions around intermediate- and high-mass young stars using mid-infrared interferometry
- Kinematic structure of massive star-forming regions - I. Accretion along filaments
- A Detailed View of the Circumstellar Environment and Disk of the Forming O-star AFGL 4176
- A multi-wavelength interferometric study of the massive young stellar object IRAS 13481-6124
- Unveiling the near-infrared structure of the massive-young stellar object NGC 3603 IRS 9A with sparse aperture masking and spectroastrometry