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Massive Black Hole Binary Evolution
Coalescence of binary supermassive black holes (SBHs) would constitute the strongest sources of gravitational waves to be observed by LISA. While the formation of binary SBHs during galaxy mergers is almost inevitable, coalescence requires that the ...
Merritt David, Milosavljević Miloš
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Accretion discs in T Tauri stars and interacting binaries [PDF]
Philip J. Armitage
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Type Icn supernovae (SNe Icn) are a newly detected, rare subtype of interacting stripped-envelope supernovae that show narrow P Cygni lines of highly ionized carbon, oxygen, and neon in their early spectra due to the interactions of the SNe ejecta with ...
Chengyuan Wu+8 more
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The Formation of Black Holes in Non-interacting, Isolated Binaries. Gaia Black Holes as Calibrators of Stellar Winds From Massive Stars [PDF]
Matthias U. Kruckow+12 more
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Cross-sections for planetary systems interacting with passing stars and binaries [PDF]
Gongjie Li, Fred C. Adams
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Effective-one-body multipolar waveform for tidally interacting binary neutron stars up to merger [PDF]
Sarp Akçay+5 more
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Modeling the Dynamics of Tidally Interacting Binary Neutron Stars up to the Merger
Sebastiano Bernuzzi+3 more
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Massive Stars in Interacting Binaries - Investigating the Progenitors of Gamma-ray Bursts [Slides]
Ayanah Cason
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