activity
20162026
most citedThe R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds

119 citations · 1.2k across the 38 of their papers we have counts for

collaborators
Showing 2024Show all

5 papers · 1 filter

astro-ph.SR2024★ 11 cited

The IACOB project XIII. Helium enrichment in O-type stars as a tracer of past binary interaction

C. Martínez-Sebastián, S. Simón-Díaz, H. Jin +4

There is increasing evidence that single-star evolutionary models are inadequate to reproduce all observational properties of massive stars. Binary interaction has emerged as a key…

astro-ph.SR2024

RAMBO I: Project introduction and first results with uGMRT

Z. Keszthelyi, K. Kurahara, Y. Iwata +4

Magnetic hot stars can emit both coherent and incoherent non-thermal radio emission. Understanding the nature of these emissions and their connection to stellar rotation and magnet…

astro-ph.SR2024

The effects of surface fossil magnetic fields on massive star evolution: V. Models at low metallicity

Z. Keszthelyi, J. Puls, G. Chiaki +4

At metallicities lower than that of the Small Magellanic Cloud, it remains essentially unexplored how fossil magnetic fields, forming large-scale magnetospheres, could affect the e…

astro-ph.SR2024★ 37 cited

Binarity at LOw Metallicity (BLOeM): a spectroscopic VLT monitoring survey of massive stars in the SMC

T. Shenar, J. Bodensteiner, H. Sana +74

Surveys in the Milky Way and Large Magellanic Cloud revealed that the majority of massive stars will interact with companions during their lives. However, knowledge of the binary p…

astro-ph.SR2024★ 18 cited

The IACOB project XI. No increase of mass-loss rates over the bistability region

Abel de Burgos, Zsolt Keszthelyi, Sergio Simón-Díaz +1

The properties of blue supergiants are key for constraining the end of the main sequence (MS) of massive stars. Whether the observed drop in the relative number of fast-rotating st…