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Table of contents
1 A journey through the interstellar medium
1.1 The three-phase model of the interstellar medium
1.2 The lifecycle of dust
1.3 Thesis organization
2 Evidence for Dust in the Universe
2.1 Dust extinction
2.2 Dust emission
2.3 Cosmic abundance of elements
2.4 Dust models
2.5 The Jones et al. (2013) dust model
3 Dust processing in the Universe
3.1 Photon – grain interaction
3.2 Atom / ion – grain interactions
3.3 Electron – grain interactions
3.4 Grain charging
3.5 Grain – grain interactions
4 Dust destruction and heating in a hot gas
4.1 Thermal sputtering
4.2 Dust heating in a hot gas
4.3 Conclusions
4.A Upgrades to DustEM
4.B Collisional cascade model
5 Evidence for collisional heated dust?
5.1 The Eyes Galaxies
5.2 PACS to SPIRE convolution
5.3 Conclusions and perspective
5.A Rigorous error estimation
5.B Hot gas cooling
6 A re-evaluation of dust processing in supernova shock waves
6.1 A supernova explosion: the different stages
6.2 Dust destruction and formation
6.3 The GRASH code
6.4 Results
6.5 Discussion
6.6 Conclusions
6.A Properties of the skewed Maxwellian distribution
7 Ram pressure stripping dynamics
7.1 Introduction
7.2 The mechanism of ram pressure stripping
7.3 Common properties of ram pressure stripped cluster galaxies
7.4 Relevant observations of ram pressure stripped galaxies
7.5 Numerical simulations
7.6 Can molecular gas be formed in the tail?
8 Conclusions and perspectives
8.1 Conclusions
8.2 Perspective
8.3 Papers related to this PhD study
