activity
20242026
collaborators

7 papers

astro-ph.SR2026

Ongoing and Post-Mass-Transfer Binaries: A Living Catalog and Unified Review of Binary Mass Transfer Products

Lieke A. C. van Son, Natsuko Yamaguchi, Pranav Nagarajan +6

Mass transfer is arguably the most defining interaction in binary stellar systems, yet many aspects of its physics remain poorly understood, from stability to endpoints and observa…

astro-ph.SR2025

Good things always come in 3s: trimodality in the binary black-hole chirp-mass distribution supports bimodal black-hole formation

Reinhold Willcox, Fabian R. N. Schneider, Eva Laplace +7

The latest GWTC-4 release from the LIGO-Virgo-KAGRA (LVK) collaboration nearly doubles the known population of double compact object mergers and reveals a new trimodal structure in…

astro-ph.SR2025

Complex spectral variability and hints of a luminous companion in the Be star + black hole binary candidate ALS 8814

Kareem El-Badry, Matthias Fabry, Hugues Sana +2

The emission-line binary ALS 8814 was recently proposed as a Be star + black hole (BH) binary based on large-amplitude radial velocity (RV) variations of a Be star and non-detectio…

astro-ph.IM2025

New Frontiers in the Study of Magnetic Massive Stars with the Habitable Worlds Observatory

Alexandre David-Uraz, Véronique Petit, Coralie Neiner +10

High-mass stars are notable for several reasons: they are characterized by strong winds, which inject momentum and enriched material into their surroundings, and die spectacularly…

astro-ph.SR2025

Characterisation of B-type stars in four young Galactic open clusters. I. Stellar content and binary properties

Federica Nardini, Julia Bodensteiner, Hugues Sana +3

Multiplicity among massive stars represents a major uncertainty in stellar evolution theory, because the extra physical processes that it introduces significantly impacts each star…

astro-ph.SR2024

Modeling contact binaries, III. Properties of a population of close, massive binaries

Matthias Fabry, Pablo Marchant, Norbert Langer +1

Among massive stars, binary interaction is the rule rather than the exception. The closest binaries, those with periods of less than about 10 days, undergo mass transfer during cor…