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Pulsational pair-instability supernovae in very close binaries
Pablo Marchant, Mathieu Renzo, Robert Farmer +4
Pair-instability and pulsational pair-instability supernovae (PPISN) have not been unambiguously observed so far. They are, however, promising candidates for the progenitors of the…
On the Origin of Black Hole Spin in High-mass X-Ray Binaries
Ying Qin, Pablo Marchant, Tassos Fragos +2
Black hole (BH) spins in low-mass X-ray binaries (LMXBs) cover a range of values that can be explained by accretion after BH birth. In contrast, the three BH spin measurements in h…
Progenitors of Type IIb Supernovae: I. Evolutionary Pathways and Rates
Niharika Sravan, Pablo Marchant, Vassiliki Kalogera
Type IIb supernovae (SNe) are important candidates to understand mechanisms that drive the stripping of stripped-envelope (SE) supernova (SN) progenitors. While binary interactions…