activity
20162024
most citedThe Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products

133 citations · 744 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2024129 cited

Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry

Gaia Collaboration, P. Panuzzo, T. Mazeh +412

Gravitational waves from black-hole merging events have revealed a population of extra-galactic BHs residing in short-period binaries with masses that are higher than expected base…

astro-ph.SR202436 cited

A magnetic massive star has experienced a stellar merger

A. J. Frost, H. Sana, L. Mahy +13

Massive stars (those larger than 8 solar masses at formation) have radiative envelopes that cannot sustain a dynamo, the mechanism that produces magnetic fields in lower-mass stars…

astro-ph.SR2023

Gaia Focused Product Release: Radial velocity time series of long-period variables

Gaia Collaboration, M. Trabucchi, N. Mowlavi +403

The third Gaia Data Release (DR3) provided photometric time series of more than 2 million long-period variable (LPV) candidates. Anticipating the publication of full radial-velocit…

astro-ph.SR202314 cited

Constraints on the multiplicity of the most massive stars known: R136 a1, a2, a3, and c

T. Shenar, H. Sana, P. A. Crowther +5

The most massive stars known to date are R 136 a1, a2, a3, and c within the central cluster R 136a of the Tarantula nebula in the Large Magellanic Cloud (LMC), with reported masses…

astro-ph.SR202319 cited

Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries

K. Sen, N. Langer, D. Pauli +6

Massive star feedback affects the evolution of galaxies, where the most massive stars may have the largest impact. The majority of massive stars are born as members of close binary…

astro-ph.SR202314 cited

Multiplicity of northern bright O-type stars with optical long baseline interferometry

Cyprien Lanthermann, Jean-Baptiste Le Bouquin, Hugues Sana +16

The study of the multiplicity of massive stars gives hints on their formation processes and their evolutionary paths, which are still not fully understood. Large separation binarie…