collaborators

9 papers

astro-ph.SR2026

The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars

C. Martínez-Sebastián, R. Gamen, O. G. Benvenuto +6

For decades, the origin of helium enrichment in O-type stars has remained an open question. In this study, we investigate the correlation between surface helium abundance and orbit…

astro-ph.SR2026

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry

K. Thomson-Paressant, D. M. Bowman, F. Nardini +16

A wide range of variability mechanisms exist among intermediate mass and massive stars, which are not yet fully understood. Using complementary data sources for a large population…

astro-ph.SR2026

SpecFANN: Spectral Fitting via Artificial Neural Networks I. A deep learning based fastwind emulator and fitting suite

M. Abdul-Masih, C. Hawcroft, T. Lechien +14

The importance of massive stars cannot be overstated: they are powerful probes of the early universe, play a vital role in the chemical and mechanical evolution of their host envir…

astro-ph.SR2026

ISOSCELES Project: II. Modelling galactic B-type stars for fast and slow wind regimes

N. Machuca, M. Curé, I. Araya +5

Radiation-driven winds in B-type stars play a key role in their evolution, yet their hydrodynamical structure remains uncertain, particularly in evolved objects. While the classica…

astro-ph.IM2026

Massive Stars in the Thirties: awaiting new Hubble discoveries

Lidia M. Oskinova, Sylvia Ekström, Miriam Garcia +4

Massive stars play a fundamental role in shaping the evolution of galaxies through feedback, chemical enrichment, and their end products as neutron stars and black holes. Despite m…

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…