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plus à gauche, montre les nuages où sont présents les amas stellaires les plus jeunes et de plus grande masse (symbolisés par des étoiles) L'image VLT à droite montre, elle, l'énergie rayonnée par les nuages. La source compacte brillante dans cette image (le pic de couleur rouge) est présente là où deux masses de gaz à des vitesses très différentes (couleurs rouge et bleue dans le cadre en bas à droite) se rencontrent. Les observations montrent que c'est là que la dissipation d'énergie est la plus forte et que les conditions sont réunies pour former un nouvel amas en quelques millions d'années. ©IAS Bibliographie ALMA CO and VLT/SINFONI H2 observations of the Antennae overlap region: mass and energy dissipation, pp.9-154 ,
Press Releases and Outreach www.cnrs.fr Contact Chercheur CNRS François Boulanger I T 01 69 85 85 73 I francois ,
l marcelino.nuno@cnrs-dir.fr GMC Giant Molecular Cloud HST Hubble Space Telescope IRAS Infrared Astronomical Satellite ISM Interstellar Medium ,
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