3D Line Radiative Transfer & Synthetic Observations with Magritte
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Amit Kumar Srivastava | L. Decin | J. Bolte | J. Yates | J. Hetherington | W. Homan | F. D. Ceuster | T. Ceulemans | Peter Boyle
[1] L. Decin,et al. SPH modelling of wind-companion interactions in eccentric AGB binary systems , 2021, Astronomy & Astrophysics.
[2] L. Decin,et al. SPH modelling of companion-perturbed AGB outflows including a new morphology classification scheme , 2021, 2107.00505.
[3] L. Decin. Evolution and Mass Loss of Cool Aging Stars: A Daedalean Story , 2020, Annual Review of Astronomy and Astrophysics.
[4] James Hetherington,et al. magritte, a modern software library for 3D radiative transfer – II. Adaptive ray-tracing, mesh construction, and reduction , 2020, Monthly Notices of the Royal Astronomical Society.
[5] I. McDonald,et al. (Sub)stellar companions shape the winds of evolved stars , 2020, Science.
[6] L. Decin,et al. Wind morphology around cool evolved stars in binaries , 2020, Astronomy & Astrophysics.
[7] James Hetherington,et al. magritte, a modern software library for 3D radiative transfer: I. Non-LTE atomic and molecular line modelling , 2019, 1912.08445.
[8] Ulrich M. Noebauer,et al. Monte Carlo radiative transfer , 2019, Living Reviews in Computational Astrophysics.
[9] B. Whitney,et al. Monte Carlo radiative transfer , 2011, 1104.4990.