activity
19982026
most citedA natural explanation for periodic X-ray outbursts in Be/X-ray binaries

312 citations · 6.5k across the 153 of their papers we have counts for

collaborators

155 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.SR2024

Astro+: Design, construction, and scientific exploitation of a large-scale massive star spectroscopic database

Klaus Rubke, Amparo Marco, Ignacio Negueruela +4

Massive stars condition the evolution of the interstellar medium by the amount of energy released during their lives and especially by their deaths as supernova explosions. The vas…

astro-ph.SR2023★ 24 cited

The IACOB project IX. Building a modern empirical database of Galactic O9-B9 supergiants: sample selection, description, and completeness

Abel de Burgos, Sergio Simón-Díaz, Miguel A. Urbaneja +1

Blue supergiants (BSGs) are important objects to study the intermediate phases of massive star evolution, helping to constrain evolutionary models. However, the lack of a holistic…

astro-ph.SR2023★ 4 cited

Gaia colour-magnitude diagrams of young open clusters: Identification in the UBC catalogue and a comparison of manual and automated analysis

Ignacio Negueruela, Abel de Burgos

Automated analysis of Gaia astrometric data has led to the discovery of many new high-quality open cluster candidates. With a good determination of their parameters, these objects…

astro-ph.SR2023★ 13 cited

Gaia-ESO Survey: massive stars in the Carina Nebula. A new census of OB stars

S. R. Berlanas, J. Maíz Apellániz, A. Herrero +16

The Gaia-ESO survey sample of massive OB stars in the Carina Nebula consists of 234 stars. The addition of brighter sources from the Galactic O-Star Spectroscopic Survey and additi…

astro-ph.IM2022★ 211 cited

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Shoko Jin, Scott C. Trager, Gavin B. Dalton +212

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree…