Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2011-04-18
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
18 pages, 11 figures
Scientific paper
In order to investigate whether massive stars form similarly to their low-mass counterparts, we have used the standard envelope plus disc geometry successfully applied to low-mass protostars to model the near-IR to sub-millimetre SED and several mid-IR images of the embedded massive star IRAS20126+4104. We have used a Monte Carlo radiative transfer dust code to model the continuum absorption, emission and scattering through two azimuthally symmetric dust geometries, the first consisting of a rotationally flattened envelope with outflow cavities, and the second which also includes a flared accretion disc. Our results show that the envelope plus disc model reproduces the observed SED and images more accurately than the model without a disc, although the latter model more closely reproduces the morphology of the mid-IR emission within a radius of 1.1" or ~1800au. We have put forward several possible causes of this discontinuity, including inner truncation of the disc due to stellar irradiation, or precession of the outflow cavity. Our best fitting envelope plus disc model has a disc radius of 9200 au. We find that it is unlikely that the outer regions of such a disc would be in hydrostatic or centrifugal equilibrium, however we calculate that the temperatures within the disc would keep it stable to fragmentation.
Johnston Katharine G.
Keto Eric
Robitaille Thomas P.
Wood Kenneth
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