activity
20022020
most citedThe VLT-FLAMES Tarantula Survey I: Introduction and observational overview

287 citations · 424 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2020★ 8 cited

The VLT-FLAMES Tarantula Survey XXXII. Low-luminosity late O-type stars -- classification, main physical parameters, and silicon abundances

N. Markova, J. Puls, P. L. Dufton +6

Analysis of late O-type stars observed in the Large Magellanic Cloud (LMC) by the VLT-FLAMES Tarantula Survey (VFTS) revealed a discrepancy between the physical properties estimate…

astro-ph.SR2017★ 89 cited

The VLT-FLAMES Tarantula Survey XXIV. Stellar properties of the O-type giants and supergiants in 30 Doradus

O. H. Ramírez-Agudelo, H. Sana, A. de Koter +21

The Tarantula region in the Large Magellanic Cloud contains the richest population of spatially resolved massive O-type stars known so far. This unmatched sample offers an opportun…

astro-ph.SR2011★ 287 cited

The VLT-FLAMES Tarantula Survey I: Introduction and observational overview

C. J. Evans, W. D. Taylor, V. Henault-Brunet +39

The VLT-FLAMES Tarantula Survey (VFTS) is an ESO Large Programme that has obtained multi-epoch optical spectroscopy of over 800 massive stars in the 30 Doradus region of the Large…

astro-ph.SR2011★ 37 cited

The VLT-FLAMES Tarantula Survey II: R139 revealed as a massive binary system

W. D. Taylor, C. J. Evans, H. Sana +22

We report the discovery that R139 in 30 Doradus is a massive spectroscopic binary system. Multi-epoch optical spectroscopy of R139 was obtained as part of the VLT-FLAMES Tarantula…

astro-ph.CO2011

The FLAMES Tarantula Survey

N. Markova, C. Evans, N. Bastian +30

The Tarantula survey is an ESO Large Programme which has obtained multi-epochs spectroscopy of over 800 massive stars in the 30 Dor region in the Large Magelanic Cloud. Here we bri…

astro-ph2002★ 3 cited

Properties of the PCygni wind found using the Self Absorption Curve method

G. Muratorio, N. Markova, M. Friedjung +1

We have used the optical lines of N II and Fe III to study the wind of the luminous blue variable P Cyg. This was performed by applying a version of the Self Absorption Curve (SAC)…