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Low Mach Number Simulation of Core Convection in Massive Stars
, 2012 Candace Gilet
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A binary merger product as the direct progenitor of a Type II-P supernova
Niu* Z +17 more
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The dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant
Munoz-Sanchez G +10 more
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Twinkle little stars: Massive stars are quenched in strong magnetic fields
Proceedings of the International Astronomical Union, 2018The role of the magnetic fields in the formation and quenching of stars with different mass is unknown. We studied the energy balance and the star formation efficiency in a sample of molecular clouds in the central kpc region of NGC 1097, known to be ...
F. Tabatabaei +2 more
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Massive stars as major factories of Galactic cosmic rays
Nature Astronomy, 2018The identification of the main contributors to the locally observed fluxes of cosmic rays is a prime objective in the resolution of the long-standing enigma of the source of cosmic rays.
F. Aharonian +2 more
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Stellar mergers as the origin of magnetic massive stars
Nature, 2019About ten per cent of ‘massive’ stars (those of more than 1.5 solar masses) have strong, large-scale surface magnetic fields1–3. It has been suggested that merging of main-sequence and pre-main-sequence stars could produce such strong fields4,5, and the ...
F. Schneider +6 more
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