collaborators

9 papers

astro-ph.SR2026

The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants

Luca Sciarini, Abel de Burgos, Sophie Rosu +3

Massive stars play a fundamental role in the evolution of the Universe. Yet, several physical processes governing their evolution remain poorly constrained. Notably, the main-seque…

astro-ph.SR2026

The outer rings of SN 1987A from year 1994 to 2024: morphology, light curves, and optical to mid-infrared spectra

Sophie Rosu, Elko Gerville-Reache, Steven Thomas +14

The outer rings (ORs) of Supernova (SN) 1987A were ejected ~20000 years before the explosion. Their characterisation is crucial for constraining the properties of the progenitor of…

astro-ph.SR2026

The Beauty of k2: Probing Stellar Interiors Using Apsidal Motion. I. The Benchmark Massive Binary HD 152248

Sophie Rosu, Luca Sciarini, Sylvia Ekström +4

Over the last decades, several independent studies have shown the need for large convective boundary mixing (CBM) and convective core sizes in massive stars to reproduce a variety…

astro-ph.SR2026

Multiplicity of Massive stars in the Milky Way (M3W). I. Project description, UNWIND, application to GLS 11 448, and DIB catalog

J. Maíz Apellániz, R. C. Gamen, G. Holgado +8

(ABRIDGED BUT NOT TOO FAR) Multiplicity is ubiquitous among massive stars and its understanding is constrained by the sample of well-determined orbits. The immediate goal of M3W is…

astro-ph.IM2026

Detached eclipsing binary star science in the 2040s

Pierre F. L. Maxted, Dominic M. Bowman, Thomas G. Wilson +7

Detached eclipsing binary stars (DEBS) are currently the best source of accurate and precise fundamental stellar parameters. This makes DEBS crucial targets for constraining the im…

astro-ph.SR2026

Chemical evolution of close massive binaries -- tidally-enhanced or tidally-suppressed mixing?

Luca Sciarini, Sophie Rosu, Sylvia Ekström +3

One of the largest source of uncertainties in the predictions of stellar models comes from the internal transport mechanisms. In close massive binaries, previous theoretical studie…