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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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Showing 2025Show all

5 papers · 1 filter

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…

astro-ph.SR2025

Hidden massive eclipsing binaries in red supergiant systems: The hierarchical triple system KQ Puppis and other candidates

D. Jadlovský, L. Molnár, A. Ercolino +26

The majority of massive stars are part of binary systems that may interact during their evolution. However, not many RSGs are known binaries, and only a few have constrained orbita…

astro-ph.SR2025★ 14 cited

Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models

X. -T. Xu, C. Schürmann, N. Langer +13

Context. The majority of massive stars are born with a close binary companion. How this affects their evolution and fate is still largely uncertain, especially at low metallicity.…

astro-ph.SR2025★ 23 cited

Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae

Andrea Ercolino, Harim Jin, Norbert Langer +1

Stripped-envelope supernovae (SNe) are H-poor transients produced at the end of the life of massive stars that previously lost their H-rich envelope. Their progenitors are thought…