Manuel Arca-Sedda

HENIZE 2-10: THE ONGOING FORMATION OF A NUCLEAR STAR CLUSTER AROUND A MASSIVE BLACK HOLE

The central region of the galaxy Henize 2-10 has a central black hole (BH) with a mass of about

Gamma-ray and X-ray emission from the Galactic centre: hints on the nuclear star cluster formation history

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The MEGaN project – I. Missing formation of massive nuclear clusters and tidal disruption events by star clusters–massive black hole interactions

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Gravitational wave sources from inspiralling globular clusters in the Galactic Centre and similar environments

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The interaction between supermassive black holes and globular clusters

. While this black hole does not appear to coincide with any central stellar over density, it is surrounded by 11 young massive clusters with masses above

The local effect of Dark Energy in galaxy clusters

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The globular cluster migratory origin of nuclear star clusters

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The MEGaN project II. Gravitational waves from intermediate mass- and binary black holes around a supermassive black hole

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Ordering the chaos: stellar black hole mergers from non-hierarchical triples

. The availability of high quality data on the structure of the galaxy and the age and mass of the clusters provides excellent initial conditions for studying the dynamical evolution of Henize 2-10s nucleus. Here we present a set of

Will a nuclear stellar disk form in the galaxy Henize 2-10?

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