Estelle Pons - LAM - Marseille Central sources in galaxies are observed as active galactic nuclei (AGN) when its supermassive black hole (SMBH) grows through a phase of significant mass accretion. They span a wide range of wavelengths, emitting from the radio to the X-rays but all are driven by the same power which is […]

Nicolás Cuello - IPAG - Grenoble What is the impact of stellar multiplicity on planet formation? This question is motivated by the fact that the process of stellar formation leads to a very high fraction of multiplicity. On top of this, planet formation occurs early on around young stellar objects. This leads to an unavoidable […]