collaborators

6 papers

astro-ph.SR2026

Astro+ database. I. Description and first results

K. Rübke, A. Marco, I. Negueruela +4

The vast amounts of spectroscopic data for massive stars provided by previous and existing instruments on ground-based and space-based telescopes have saturated our capability to p…

astro-ph.SR2026

The IACOB project: XVI. Surface helium abundances in Galactic O-type stars: indications for identifying binary interaction products

S. Simón-Díaz, G. Holgado, C. Martínez-Sebastián +13

The presence of massive O-type stars with surfaces enriched by CNO-cycle products has been known since the early 1980s. For many years, internal rotational mixing was assumed to be…

astro-ph.SR2026

Binarity at LOw Metallicity (BLOeM): Projected rotational velocities

D. J. Lennon, S. R. Berlanas, A. Herrero +36

The Binarity at LOw Metallicity (BLOeM) survey is an ESO large programme designed to obtain multi-epoch spectroscopy for 929 massive stars in the Small Magellanic Cloud (SMC). It w…

astro-ph.SR2025

Probing Thin Winds in Massive OB Stars of the SMC with JWST/NIRSPEC Br-alpha Spectroscopy

Miriam Garcia, Alexander W. Fullerton, Francisco Najarro +12

Mass loss is a key physical process in the evolution of massive stars, the impact of which propagates into galactic evolution, population synthesis models, the interpretation of hi…

astro-ph.SR2025

X-Shooting ULLYSES: massive stars at low metallicity: XII. The clumped winds of O-type (super)giants in the Large Magellanic Cloud

Sarah A. Brands, Frank Backs, Alex de Koter +23

Mass loss governs the evolution of massive stars and shapes the stellar surroundings. To quantify the impact of the stellar winds we need to know the exact mass-loss rates; however…

astro-ph.SR2025

A reference framework for extremely metal-poor OB star studies: calibrations for stellar parameters and intrinsic colours

Marta Lorenzo, Miriam Garcia, Norberto Castro +4

We provide the first reference framework for extremely metal-poor (XMP) OB-type stars. We parsed a grid of 0.10 FASTWIND models, covering the parameter space of O stars…