Context. The star cluster R136 inside the Large Magellanic Cloud hosts a rich population of
massive stars, including the most massive stars known. The strong stellar winds of these …

The sharpest optical images of the R136 cluster in the Large Magellanic Cloud are
presented, allowing us for the first time to resolve members of the central core, including …

We report the identification of very massive stars (VMS; mass> 100 M⊙) that may be
segregated in the center of the young massive star cluster at z= 2.37 hosted in the lensed …

We reassess the historical LX/L Bol relation for early-type stars from a comparison between
T-ReX, the Chandra ACIS X-ray survey of the Tarantula Nebula in the Large Magellanic …

Context. The cluster R136 in the giant star-forming region 30 Doradus in the Large
Magellanic Cloud (LMC) offers a unique opportunity to resolve a stellar population in a …

Measuring the orbits of directly imaged exoplanets requires precise astrometry at the
milliarcsec level over long periods of time due to their wide separation to the stars (≳ 10 au) …

Mass segregation is seen in many star clusters, but whether massive stars form in the center
of a cluster or migrate there dynamically is still debated. N-body simulations have shown that …

We compared high-contrast near-infrared images of the core of R136 taken by
VLT/SPHERE, in two epochs separated by 3.06 years. For the first time we monitored the …

Polarimetry continues to be a very active field, be it in terms of research papers, meetings,
instruments and research programs. This was particularly true from March 2018 through …