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Interacting supernovae from wide massive binary systems
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The impact of periastron passage on the X-ray and optical properties of the Symbiotic System R Aquarii
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Influence of a mass transfer stability criterion on double white dwarf populations
Astrophysics with the Laser Interferometer Space Antenna
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3D simulations of AGB stellar winds
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The 2020 Eclipse of R Aquarii in the Near-infrared: Mid-eclipse Observations of Disk Distress
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A gap in the double white dwarf separation distribution caused by the common-envelope evolution: astrometric evidence from Gaia
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New Clues to the Evolution of Dwarf Carbon Stars From Their Variability and X-Ray Emission
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Binary Interaction Dominates Mass Ejection in Classical Novae
Wide binary pulsars from electron-capture supernovae
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Dynamical Effects of Colliding Outflows in Binary Systems
Raman-scattered O vi Features in the Symbiotic Nova RR Telescopii
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The formation of barium giants via mass accretion in binary systems
(Sub)stellar companions shape the winds of evolved stars
L. Decin, M. Montargès, A. M. S. Richards, C. A. Gottlieb, W. Homan, I. McDonald, I. El Mellah, T. Danilovich, S. H. J. Wallström, A. Zijlstra, A. Baudry, J. Bolte, E. Cannon, E. De Beck, F. De Ceuster, A. de Koter, J. De Ridder, S. Etoka, D. Gobrecht, M. Gray, F. Herpin, M. Jeste, E. Lagadec, P. Kervella, T. Khouri, et al. Science 369(6510) 1497 (2020) https://doi.org/10.1126/science.abb1229
Multi-scale high-performance computing in astrophysics: simulating clusters with stars, binaries and planets
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Spectral analysis of the barium central star of the planetary nebula Hen 2−39