Speaker
Illia Bilinskyi
(Taras Shevchenko National University of Kyiv, Akademika Hlushkova Ave, 4, Kyiv, Ukraine, 03022)
Description
We present the result of modelling of spectral energy distribution of the infrared source IRAS 22150+6109. The object emits an excess of radiation in far infrared band. It was interpreted to be a young massive pre-main-sequence star and the protoplanetary disk on late stage. We use radiative transfer code RADMC-3D for the simulations of spectral energy distribution. The code itself implements the Monte-Carlo ray tracing method with spherical grid fragmentation. We performed simulations and obtained best-fit parameters for the model of the protoplanetary disk. The investigation of such objects will help to understand protoplanetary disks emission better.
Primary authors
Illia Bilinskyi
(Taras Shevchenko National University of Kyiv, Akademika Hlushkova Ave, 4, Kyiv, Ukraine, 03022)
Olga Zakhozhay
(Main Astronomical Observatory National Academy of Sciences of Ukraine)
Dr
Peter Berczik
(Main Astronomical Observatory National Academy of Sciences of Ukraine)
