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20122026
most citedThe VLT-FLAMES Tarantula Survey VIII. Multiplicity properties of the O-type star population

530 citations · 1.9k across the 19 of their papers we have counts for

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astro-ph.SR2021★ 42 cited

The B-type Binaries Characterisation Programme I. Orbital solutions for the 30 Doradus population

J. I. Villaseñor, W. D. Taylor, C. J. Evans +6

We present results from the B-type Binaries Characterisation (BBC) programme, a multi-epoch spectroscopic study of 88 early B-type binary candidates in the 30 Doradus region of the…

astro-ph.SR2018

ELT Spectroscopy of Extragalactic Massive Stars

C. J. Evans, O. H. Ramirez-Agudelo, M. Garcia +2

Quantitative spectroscopy of O-type stars in galaxies beyond 1 Mpc requires the unprecedented sensitivity of the so-called Extremely Large Telescopes. Visible spectroscopy with the…

astro-ph.SR2018★ 79 cited

Response to comment on "An excess of massive stars in the local 30 Doradus starburst"

F. R. N. Schneider, H. Sana, C. J. Evans +29

Farr and Mandel reanalyse our data, finding initial-mass-function slopes for high mass stars in 30 Doradus that agree with our results. However, their reanalysis appears to underpr…

astro-ph.SR2018★ 103 cited

The VLT-FLAMES Tarantula Survey. XXIX. Massive star formation in the local 30 Doradus starburst

F. R. N. Schneider, O. H. Ramírez-Agudelo, F. Tramper +24

The 30 Doradus (30 Dor) nebula in the Large Magellanic Cloud (LMC) is the brightest HII region in the Local Group and a prototype starburst similar to those found in high redshift…

astro-ph.SR2018★ 34 cited

The VLT-FLAMES Tarantula Survey: XXVIII. Nitrogen abundances for apparently single dwarf and giant B-type stars with small projected rotational velocities

P. L. Dufton, A. Thompson, P. A. Crowther +13

Previous analyses of the spectra of OB-type stars in the Magellanic Clouds have identified targets with low projected rotational velocities and relatively high nitrogen abundances.…

astro-ph.SR2018★ 263 cited

An excess of massive stars in the local 30 Doradus starburst

F. R. N. Schneider, H. Sana, C. J. Evans +29

The 30 Doradus star-forming region in the Large Magellanic Cloud is a nearby analogue of large star-formation events in the distant Universe. We determine the recent formation hist…

astro-ph.SR2017★ 59 cited

The VLT-FLAMES Tarantula Survey XXVI: Properties of the O-dwarf population in 30 Doradus

C. Sabín-Sanjulián, S. Simón-Díaz, A. Herrero +21

The VLT-FLAMES Tarantula Survey has observed hundreds of O-type stars in the 30 Doradus region of the Large Magellanic Cloud (LMC). We study the properties of 105 apparently single…

astro-ph.SR2016★ 154 cited

The Tarantula Massive Binary Monitoring: I. Observational campaign and OB-type spectroscopic binaries

L. A. Almeida, H. Sana, W. Taylor +24

Massive binaries (MBs) play a crucial role in the Universe. Knowing the distributions of their orbital parameters (OPs) is important for a wide range of topics, from stellar feedba…

astro-ph.SR2015★ 74 cited

Discovery of the massive overcontact binary VFTS 352: Evidence for enhanced internal mixing

L. A. Almeida, H. Sana, S. E. de Mink +15

The contact phase expected to precede the coalescence of two massive stars is poorly characterized due to the paucity of observational constraints. Here we report on the discovery…

astro-ph.SR2015★ 89 cited

The VLT-FLAMES Tarantula Survey XXI. Stellar spin rates of O-type spectroscopic binaries

O. H. Ramírez-Agudelo, H. Sana, S. E. de Mink +9

The initial distribution of spin rates of massive stars is a fingerprint of their elusive formation process. It also sets a key initial condition for stellar evolution and is thus…

astro-ph.SR2014★ 49 cited

The properties of ten O-type stars in the low-metallicity galaxies IC 1613, WLM and NGC 3109

F. Tramper, H. Sana, A. de Koter +2

Massive stars likely played an important role in the reionization of the Universe, and the formation of the first black holes. Massive stars in low-metallicity environments in the…

astro-ph.SR2014★ 2 cited

Rotational velocities of single and binary O-type stars in the Tarantula Nebula

O. H. Ramírez-Agudelo, H. Sana, A. de Koter +15

Rotation is a key parameter in the evolution of massive stars, affecting their evolution, chemical yields, ionizing photon budget, and final fate. We determined the projected rotat…

astro-ph.SR2013★ 57 cited

The VLT-FLAMES Tarantula Survey. XIII: On the nature of O Vz stars in 30 Doradus

C. Sabín-Sanjulián, S. Simón-Díaz, A. Herrero +13

AIMS. We test the hypothesis of O Vz stars (characterized by having HeII4686 stronger in absorption than other He lines in their blue-violet spectra) being at a younger evolutionar…

astro-ph.SR2013★ 232 cited

The VLT-FLAMES Tarantula Survey XII. Rotational velocities of the single O-type stars

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

Aims. Using ground based multi-object optical spectroscopy obtained in the framework of the VLT-FLAMES Tarantula Survey (VFTS), we aim to establish the (projected) rotational veloc…

astro-ph.SR2012★ 142 cited

The VLT-FLAMES Tarantula Survey X: Evidence for a bimodal distribution of rotational velocities for the single early B-type stars

P. L. Dufton, N. Langer, P. R. Dunstall +12

Aims: Projected rotational velocities (\vsini) have been estimated for 334 targets in the VLT-FLAMES Tarantula survey that do not manifest significant radial velocity variations an…

astro-ph.SR2012★ 530 cited

The VLT-FLAMES Tarantula Survey VIII. Multiplicity properties of the O-type star population

H. Sana, A. de Koter, S. E. de Mink +14

Aims. We analyze the multiplicity properties of the massive O-type star population. With 360 O-type stars, this is the largest homogeneous sample of massive stars analyzed to date.…