activity
20062023
most citedThe VLT-FLAMES Tarantula Survey I: Introduction and observational overview

287 citations · 723 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2023★ 41 cited

X-Shooting ULLYSES: Massive stars at low metallicity. III. Terminal wind speeds of ULLYSES massive stars

C. Hawcroft, H. Sana, L. Mahy +26

The winds of massive stars have an impact on stellar evolution and on the surrounding medium. The maximum speed reached by these outflows, the terminal wind speed, is a global wind…

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★ 106 cited

The VLT-FLAMES Tarantula Survey III: A very massive star in apparent isolation from the massive cluster R136

Joachim M. Bestenlehner, Jorick S. Vink, G. Gräfener +17

VFTS 682 is located in an active star-forming region, at a projected distance of 29 pc from the young massive cluster R136 in the Tarantula Nebula of the Large Magellanic Cloud. It…

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.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-ph2007★ 93 cited

Polarized NIR and X-ray Flares from SgrA*

A. Eckart, F. K. Baganoff, M. Zamaninasab +18

Stellar dynamics indicate the presence of a super massive 3-4x10^6 Msun solm black hole at the Galactic Center. It is associated with the variable radio, near-infrared, and X-ray c…