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Improving 1D stellar atmosphere models with insights from multi-dimensional simulations
G. González-Torà, A. A. C. Sander, J. O. Sundqvist, D. Debnath, L. Delbroek, J. Josiek, R. R. Lefever, N. Moens, C. Van der Sijpt and O. Verhamme Astronomy & Astrophysics 694 A269 (2025) https://doi.org/10.1051/0004-6361/202452241
Progress towards a 3D Monte Carlo radiative transfer code for outflow wind modelling
Chandra grating spectroscopy of embedded wind shock X-ray emission from O stars shows low plasma temperatures and significant wind absorption
David H Cohen, Winter Parts, Graham M Doskoch, et al. Monthly Notices of the Royal Astronomical Society 503(1) 715 (2021) https://doi.org/10.1093/mnras/stab270
Using Shell models to investigate clumping in the wind of the O7Iaf + supergiant AzV83
Tahina Ramiaramanantsoa, Richard Ignace, Anthony F J Moffat, et al. Monthly Notices of the Royal Astronomical Society 490(4) 5921 (2019) https://doi.org/10.1093/mnras/stz2895
Theoretical X-Ray Light Curves of Young SNe. II. The Example of SN 2013ej
Line-driven ablation of circumstellar discs – II. Analysing the role of multiple resonances
Nathaniel Dylan Kee, Stanley Owocki and Rolf Kuiper Monthly Notices of the Royal Astronomical Society 474(1) 847 (2018) https://doi.org/10.1093/mnras/stx2772
Subphotospheric fluctuations in magnetized radiative envelopes: contribution from unstable magnetosonic waves
Koushik Sen, Rodrigo Fernández and Aristotle Socrates Monthly Notices of the Royal Astronomical Society 477(2) 2286 (2018) https://doi.org/10.1093/mnras/sty736
Accretion from a clumpy massive-star wind in supergiant X-ray binaries
e-MERLIN 21 cm constraints on the mass-loss rates of OB stars in Cyg OB2
J. C. Morford, D. M. Fenech, R. K. Prinja, R. Blomme and J. A. Yates Monthly Notices of the Royal Astronomical Society 463(1) 763 (2016) https://doi.org/10.1093/mnras/stw1914
Long-wavelength, free–free spectral energy distributions from porous stellar winds
Lidia M. Oskinova, Brankica Kubátová and Wolf-Rainer Hamann Journal of Quantitative Spectroscopy and Radiative Transfer 183 100 (2016) https://doi.org/10.1016/j.jqsrt.2016.06.017
X-ray, UV and optical analysis of supergiants: ϵ Ori
Raul E. Puebla, D. John Hillier, Janos Zsargó, David H. Cohen and Maurice A. Leutenegger Monthly Notices of the Royal Astronomical Society 456(3) 2907 (2016) https://doi.org/10.1093/mnras/stv2783
A unified heuristic X-ray production model for thick and thin winds from single nonmagnetic hot stars
Roland Walter, Alexander A. Lutovinov, Enrico Bozzo and Sergey S. Tsygankov The Astronomy and Astrophysics Review 23(1) (2015) https://doi.org/10.1007/s00159-015-0082-6
The variable stellar wind of Rigel probed at high spatial and spectral resolution
UV spectral analysis of very hot H-deficient [WCE]-type central stars of planetary nebulae: NGC 2867, NGC 5189, NGC 6905, Pb 6 and Sand 3
Graziela R. Keller, Luciana Bianchi and Walter J. Maciel Monthly Notices of the Royal Astronomical Society 442(2) 1379 (2014) https://doi.org/10.1093/mnras/stu878
Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive
David H. Cohen, Emma E. Wollman, Maurice A. Leutenegger, et al. Monthly Notices of the Royal Astronomical Society 439(1) 908 (2014) https://doi.org/10.1093/mnras/stu008
Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars
Measuring the shock-heating rate in the winds of O stars using X-ray line spectra
David H. Cohen, Zequn Li, Kenneth G. Gayley, et al. Monthly Notices of the Royal Astronomical Society 444(4) 3729 (2014) https://doi.org/10.1093/mnras/stu1661
ANALYTICAL SOLUTIONS FOR RADIATION-DRIVEN WINDS IN MASSIVE STARS. I. THE FAST REGIME
A generalized porosity formalism for isotropic and anisotropic effective opacity and its effects on X-ray line attenuation in clumped O star winds
Jon O. Sundqvist, Stanley P. Owocki, David H. Cohen, Maurice A. Leutenegger and Richard H. D. Townsend Monthly Notices of the Royal Astronomical Society 420(2) 1553 (2012) https://doi.org/10.1111/j.1365-2966.2011.20141.x
X-RAY EMISSION LINE PROFILES FROM WIND CLUMP BOW SHOCKS IN MASSIVE STARS