scispace - formally typeset
M

M. A. de Avillez

Researcher at University of Évora

Publications -  21
Citations -  1021

M. A. de Avillez is an academic researcher from University of Évora. The author has contributed to research in topics: Supernova & Galaxy. The author has an hindex of 11, co-authored 21 publications receiving 954 citations. Previous affiliations of M. A. de Avillez include Technical University of Berlin.

Papers
More filters
Journal ArticleDOI

Global dynamical evolution of the ISM in star forming galaxies. I. High resolution 3D simulations: Effect of the magnetic field

TL;DR: In this paper, the role of magnetized matter circulation between the gaseous disk and the surrounding galactic halo is investigated using a 3D MHD code with adaptive mesh refinement developed for this purpose.
Journal ArticleDOI

Volume filling factors of the ISM phases in star forming galaxies. I. The role of the disk-halo interaction

TL;DR: In this article, the role of matter circulation between the disk and halo in establishing the volume filling factors of different ISM phases in the Galactic disk was investigated, using a modified version of the three-dimensional supernova-driven ISM model of Avillez (2000).
Journal ArticleDOI

Exploring cosmic origins with CORE: Survey requirements and mission design

Jacques Delabrouille, +240 more
TL;DR: The requirements for a future CMB polarisation survey addressing these scientific objectives are listed, and the design drivers of the COREmfive space mission proposed to ESA in answer to the "M5" call for a medium-sized mission are discussed.
Journal ArticleDOI

The locations of recent supernovae near the Sun from modelling 60 Fe transport

TL;DR: Calculations of the most probable trajectories and masses of the supernova progenitors, and hence their explosion times and sites, are reported and the model reproduces the measured relative abundances very well.
Journal ArticleDOI

What Physical Processes Drive the Interstellar Medium in the Local Bubble

TL;DR: In this article, the age of the Local Bubble is derived from comparison with Hi and UV absorption line data to be 14.5± 0.4 0.7 Myr, and the merging of the two bubbles in about 3 Myr from now, when the interaction shell starts to fragment.