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19962026
most citedMass-loss predictions for O and B stars as a function of metallicity

1.7k citations · 12.2k across the 150 of their papers we have counts for

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Showing 2017Show all

7 papers · 1 filter

astro-ph.SR2017★ 4 cited

The VLT-FLAMES Tarantula Survey

Jorick S. Vink, C. J. Evans, J. Bestenlehner +5

We present a number of notable results from the VLT-FLAMES Tarantula Survey (VFTS), an ESO Large Program during which we obtained multi-epoch medium-resolution optical spectroscopy…

astro-ph.GA2017★ 62 cited

The ESO Diffuse Interstellar Bands Large Exploration Survey: EDIBLES I. Project description, survey sample and quality assessment

Nick Cox, Jan Cami, Amin Farhang +27

The carriers of the diffuse interstellar bands (DIBs) are largely unidentified molecules ubiquitously present in the interstellar medium (ISM). After decades of study, two strong a…

astro-ph.HE2017★ 72 cited

Predicting the Presence of Companions for Stripped-Envelope Supernovae: The Case of the Broad-Lined Type Ic SN 2002ap

E. Zapartas, S. E. de Mink, S. D. Van Dyk +10

Many young, massive stars are found in close binaries. Using population synthesis simulations we predict the likelihood of a companion star being present when these massive stars e…

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.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.HE2017★ 188 cited

Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction

E. Zapartas, S. E. de Mink, R. G. Izzard +8

Most massive stars, the progenitors of core-collapse supernovae, are in close binary systems and may interact with their companion through mass transfer or merging. We undertake a…