First light for the EWOCS (Extensive Westerlund One Chandra Survey) project

On June 2019, the panel for the evaluation of the proposals for observations with the NASA telescope Chandra, operating in the X-rays, which met up in Boston, has approved the Large Project: “Star formation in starburst: a deep ACIS-I observation of Westerlund 1“, led by the astronomer Mario Giuseppe Guarcello – INAF Astronomical Observatory of Palermo. More details on the

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The Gaia-ESO survey and the evolution of stellar clusters. Published on A&A “The Gaia-ESO Survey: kinematical and dynamical study of four young open clusters” of L. Bravi (INAF-OA Arcetri)

Despite the stars in our Galaxy typically formed in stellar clusters, only a small fraction of them today is observed associated with a cluster. This led to the conclusion that stellar clusters typically disperse in 10-100 million years. Two mechanisms are thought to be responsible for the dispersion of stellar clusters. According to the model of the “residual gas expulsion”,

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“The Gaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon I” by G. Sacco published on Astronomy & Astrophysics

The star formation process starts with the gravitational collapse of large and cold clouds of gas and dust. Despite it sounds like a simple process, it is actually very complicated and we still lack full comprehension of the details of how these clouds can form clusters and associations of young stars.   This is one of the main objectives of

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