Cool outflows in galaxies and their implications
Neutral-atomic and molecular outflows are a common occurrence in galaxies, near and far.
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …
A review of the theory of galactic winds driven by stellar feedback
D Zhang - Galaxies, 2018 - mdpi.com
Galactic winds from star-forming galaxies are crucial to the process of galaxy formation and
evolution, regulating star formation, sha** the stellar mass function and the mass …
evolution, regulating star formation, sha** the stellar mass function and the mass …
Momentum injection by supernovae in the interstellar medium
Supernova (SN) explosions deposit prodigious energy and momentum in their
environments, with the former regulating multiphase thermal structure and the latter …
environments, with the former regulating multiphase thermal structure and the latter …
The PLUTO code for adaptive mesh computations in astrophysical fluid dynamics
A Mignone, C Zanni, P Tzeferacos… - The Astrophysical …, 2011 - iopscience.iop.org
We present a description of the adaptive mesh refinement (AMR) implementation of the
PLUTO code for solving the equations of classical and special relativistic …
PLUTO code for solving the equations of classical and special relativistic …
The launching of cold clouds by galaxy outflows. I. Hydrodynamic interactions with radiative cooling
E Scannapieco, M Brüggen - The Astrophysical Journal, 2015 - iopscience.iop.org
To better understand the nature of the multiphase material found in outflowing galaxies, we
study the evolution of cold clouds embedded in flows of hot and fast material. Using a suite …
study the evolution of cold clouds embedded in flows of hot and fast material. Using a suite …
Driving outflows with relativistic jets and the dependence of active galactic nucleus feedback efficiency on interstellar medium inhomogeneity
We examine the detailed physics of the feedback mechanism by relativistic active galactic
nucleus (AGN) jets interacting with a two-phase fractal interstellar medium (ISM) in the kpc …
nucleus (AGN) jets interacting with a two-phase fractal interstellar medium (ISM) in the kpc …
The fully developed remnant of a neutrino-driven supernova-Evolution of ejecta structure and asymmetries in SNR Cassiopeia A
S Orlando, A Wongwathanarat, HT Janka… - Astronomy & …, 2021 - aanda.org
Context. The remnants of core-collapse supernovae (SNe) are probes of the physical
processes associated with their parent SNe. Aims. Here we aim to explore to which extent …
processes associated with their parent SNe. Aims. Here we aim to explore to which extent …
Starburst-driven galactic winds: filament formation and emission processes
We have performed a series of three-dimensional simulations of the interaction of a
supersonic wind with a nonspherical radiative cloud. These simulations are motivated by our …
supersonic wind with a nonspherical radiative cloud. These simulations are motivated by our …
The launching of cold clouds by galaxy outflows. II. the role of thermal conduction
M Brüggen, E Scannapieco - The Astrophysical Journal, 2016 - iopscience.iop.org
We explore the impact of electron thermal conduction on the evolution of radiatively cooled
cold clouds embedded in flows of hot and fast material as it occurs in outflowing galaxies …
cold clouds embedded in flows of hot and fast material as it occurs in outflowing galaxies …
Inside the core of a young massive star cluster: 3D MHD simulations
DV Badmaev, AM Bykov… - Monthly Notices of the …, 2022 - academic.oup.com
Young massive star clusters inhabit regions of star formation and play an essential role in
the galactic evolution. They are sources of both thermal and non-thermal radiation, and are …
the galactic evolution. They are sources of both thermal and non-thermal radiation, and are …