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L. Images-de-droite, C. Herrera, A. Le, V. L-'image, and A. , 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

C. Appendix, Press Releases and Outreach www.cnrs.fr Contact Chercheur CNRS François Boulanger I T 01 69 85 85 73 I francois

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