activity
20202026
most citedAn Ultra-Hot Neptune in the Neptune desert

85 citations · 268 across the 17 of their papers we have counts for

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13 papers · 1 filter

astro-ph.SR2026

Binary-induced mass increase and helium enrichment of the envelopes of Type~IIP supernova progenitors

Caroline Mannes, Norbert Langer, Andrea Ercolino

Binary interactions are expected to play a major role in shaping the progenitor population of core-collapse supernovae, particularly in the era of deep, high-cadence transient surv…

astro-ph.SR2026

Progenitor models of supernovae interacting with their binary companions

Andrea Ercolino

The appearance of nearly all core-collapse (CC) supernovae (SNe) is largely affected by the interaction between their progenitors and a close binary companion. Using a comprehensiv…

astro-ph.SR2026

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models

Andrea Ercolino, Norbert Langer, Avishay Gal-Yam +6

Most massive stars live in binary systems. When the first supernova (SN) in a binary occurs, the ejecta hit the companion, which may inflate as a consequence, and then interact wit…

astro-ph.SR2026★ 5 cited

The drastic impact of Eddington-limit induced mass ejections on massive star populations

D. Pauli, N. Langer, A. Schootemeijer +6

Massive stars are the key engines of the Universe. However, their evolution and thus their ionizing feedback are still not fully understood. One of the largest gaps in current stel…

astro-ph.SR2025★ 7 cited

A comprehensive grid of massive binary evolution models for the Galaxy - Surface properties of post-mass transfer stars

Harim Jin, Norbert Langer, Andrea Ercolino +1

Massive stars often evolve in binary systems, in which binary interactions significantly affect their evolution. Massive stars in the Galaxy serve as valuable testbeds for this due…

astro-ph.SR2025★ 4 cited

The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction

Andrea Ercolino, Harim Jin, Norbert Langer +3

The observational properties of core-collapse supernovae (CC-SNe) are shaped by the envelopes of their progenitors. In massive binary systems, mass-transfer alters the pre-SN struc…