activity
20132025
most citedMassive pre-main sequence stars in M17

31 citations · 80 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2025★ 9 cited

An interferometric study of B star multiplicity

A. J. Frost, H. Sana, J-B Le Bouquin +7

Massive stars can have extreme effects on their environments from local to galactic scales. While O star multiplicity has been studied over a broad separation range (to the point w…

astro-ph.SR2022★ 30 cited

The VLT-FLAMES Tarantula Survey: Observational evidence for two distinct populations of massive runaway stars in 30 Doradus

H. Sana, O. H. Ramírez-Agudelo, V. Hénault-Brunet +17

Two main scenarios have been proposed for origin of massive runaway stars -- dynamical ejection or release from a binary at the first core collapse -- but their relative contributi…

astro-ph.SR2019★ 10 cited

The young stellar content of the giant HII regions M8, G333.6-0.2, and NGC6357 with VLT/KMOS

M. C. Ramírez-Tannus, J. Poorta, A. Bik +14

Context: The identification and characterisation of populations of young massive stars in (giant) HII regions provides important constraints on i) the formation process of massive…

astro-ph.SR2017★ 31 cited

Massive pre-main sequence stars in M17

María Claudia Ramírez-Tannus, Lex Kaper, Alex de Koter +6

The formation process of massive stars is still poorly understood. Massive young stellar objects (mYSOs) are deeply embedded in their parental clouds, they are rare and thus typica…

astro-ph.SR2013

Rotational properties of the O-type star population in the Tarantula region

O. H. Ramírez-Agudelo, S. Simón-Díaz, H. Sana +15

The 30 Doradus (30\,Dor) region in the Large Magellanic Cloud (also known as the Tarantula Nebula) is the nearest massive starburst region, containing the richest sample of massive…