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Claudio Melioli

Researcher at University of São Paulo

Publications -  40
Citations -  1956

Claudio Melioli is an academic researcher from University of São Paulo. The author has contributed to research in topics: Galaxy & Supernova. The author has an hindex of 16, co-authored 39 publications receiving 1832 citations. Previous affiliations of Claudio Melioli include University of Bologna & INAF.

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Journal ArticleDOI

Introducing the CTA concept

B. S. Acharya, +982 more
TL;DR: The Cherenkov Telescope Array (CTA) as discussed by the authors is a very high-energy (VHE) gamma ray observatory with an international collaboration with more than 1000 members from 27 countries in Europe, Asia, Africa and North and South America.
Journal ArticleDOI

The dance of heating and cooling in galaxy clusters: three-dimensional simulations of self-regulated active galactic nuclei outflows

TL;DR: In this article, a modified version of the adaptive mesh refinement code FLASH 3.2 was used to explore several feedback mechanisms that self-regulate the mechanical power of the central active nucleus.
Journal ArticleDOI

The Dance of Heating and Cooling in Galaxy Clusters: 3D Simulations of Self-Regulated AGN Outflows

TL;DR: In this article, a modified version of AMR code FLASH 3.2 was used to explore several feedback mechanisms which self-regulate the mechanical power of the ICM, and two schemes were proposed to quench cooling flow and at the same time preserve a cool core appearance for a long term evolution.
BookDOI

Magnetic Fields in Diffuse Media

TL;DR: In this article, the Atacama Large Millimeter/submillimeter Array (LME/sub-millimeter array) was used to measure the magnetic field with ground state alignment.
Journal ArticleDOI

AGN feedback in galaxy groups: the delicate touch of self-regulated outflows

TL;DR: In this article, a modified version of the adaptive mesh refinement code FLASH 3.2 has been used to simulate galaxy groups with both cold and hybrid accretion models, and it has been shown that successful 3D simulations with both models are almost convergent in the galaxy group environment.