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NGC 6752 : a globular cluster with a resolved post-collapse core ?

M. Aurière, S. Ortolani

Abstract

La photometrie CCD BV de l'amas globulaire NGC 6752 est presentee. L'exces de brillance centrale et le profil de la region centrale sont analyses. Une loi de puissance est etablie pour le profil de brillance radiale en bande V.

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Available abstract

Key concepts: Physics, Globular cluster, Astrophysics, Astronomy, Galaxy

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