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Modelling stellar evolution in mass-transferring binaries and gravitational-wave progenitors with METISSE
Poojan Agrawal, Jarrod Hurley, Simon Stevenson +3
Massive binaries are vital sources of various transient processes, including gravitational-wave mergers. However, large uncertainties in the evolution of massive stars, both physic…
A systematic study of super-Eddington layers in the envelopes of massive stars
Poojan Agrawal, Simon Stevenson, Dorottya Szécsi +1
The proximity to the Eddington luminosity has been attributed as the cause of several observed effects in massive stars. Computationally, if the luminosity carried through radiatio…
Explaining the differences in massive star models from various simulations
Poojan Agrawal, Dorottya Szécsi, Simon Stevenson +2
The evolution of massive stars is the basis of several astrophysical investigations, from predicting gravitational-wave event rates to studying star-formation and stellar populatio…
The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
Poojan Agrawal, Jarrod Hurley, Simon Stevenson +2
In the era of advanced electromagnetic and gravitational wave detectors, it has become increasingly important to effectively combine and study the impact of stellar evolution on bi…
BSE versus StarTrack: implementations of new wind, remnant-formation, and natal-kick schemes in NBODY7 and their astrophysical consequences
Sambaran Banerjee, Krzysztof Belczynski, Christopher L. Fryer +4
The masses of stellar-remnant black holes (BH), as a result of their formation via massive single- and binary-stellar evolution, is of high interest in this era of gravitational-wa…
No cataclysmic variables missing: higher merger rate brings into agreement observed and predicted space densities
Diogo Belloni, Matthias R. Schreiber, Mónica Zorotovic +4
The predicted and observed space density of cataclysmic variables (CVs) have been for a long time discrepant by at least an order of magnitude. The standard model of CV evolution p…