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Disk Wind Feedback from High-mass Protostars. III. Synthetic CO Line Emission
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Accuracy of ALMA estimates of young disk radii and masses
Ngo-Duy Tung, Leonardo Testi, Ugo Lebreuilly, Patrick Hennebelle, Anaëlle Maury, Ralf S. Klessen, Luca Cacciapuoti, Matthias González, Giovanni Rosotti and Sergio Molinari Astronomy & Astrophysics 684 A36 (2024) https://doi.org/10.1051/0004-6361/202348730
Spectroscopic and photometric studies on four solar-type short-period contact binaries in the triple stellar systems
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3D radiative transfer modelling and virial analysis of starless cores in the B10 region of the Taurus molecular cloud
Samantha Scibelli, Yancy Shirley, Anika Schmiedeke, Brian Svoboda, Ayushi Singh, James Lilly and Paola Caselli Monthly Notices of the Royal Astronomical Society 521(3) 4579 (2023) https://doi.org/10.1093/mnras/stad827
Improving Monte Carlo radiative transfer simulations: A shift of framework
Modeling Nitrogen Fractionation in the Protoplanetary Disk around TW Hya: Model Constraints on Grain Population and Carbon-to-oxygen Elemental Abundance Ratio
Observational signatures of outbursting protostars - I: From hydrodynamic simulations to observations
Benjamin MacFarlane, Dimitris Stamatellos, Doug Johnstone, et al. Monthly Notices of the Royal Astronomical Society 487(4) 5106 (2019) https://doi.org/10.1093/mnras/stz1512
Massive dust clumps in the envelope of the red supergiant VY Canis Majoris
Large-scale magnetic field in the accretion discs of young stars: the influence of magnetic diffusion, buoyancy and Hall effect
S. A. Khaibrakhmanov, A. E. Dudorov, S. Yu. Parfenov and A. M. Sobolev Monthly Notices of the Royal Astronomical Society 464(1) 586 (2017) https://doi.org/10.1093/mnras/stw2349
The physical and chemical structure of Sagittarius B2