Shock waves are known to significantly alter the medium through with they propagate. Shocks in the interstellar medium have been known to affect star formation. Likewise, shocks in the intergalactic medium are expected to affect galaxy formation and the confinement of intergalactic clouds. Because of their significant influence, it is important to have a sound understanding of the different solutions used to study shocks and see how they differ. In this paper, I will focus on the self similar solution, thoroughly developed by Ostriker and McKee, and the explosion model, developed by Tegmark, Silk, and Evrard
Supernovae launch spherical shocks into the circumstellar medium (CSM). These shocks may interact wi...
We study the properties of cosmological shock waves identified in high-resolution, N-body/hydrodynam...
Understanding the causes and effects of explosions is important to experts in a broad range of disci...
Shock waves form in the intergalactic medium (IGM) as a consequence of accretion, merger, and turbul...
Cosmological shock waves are induced during hierarchical formation of large-scale structure in the u...
Bubbles in the interstellar medium are produced by astrophysical sources, which continuously or expl...
Star formation in general, and starbursts in particular, drive the evolution of galaxies. To underst...
Like in our galaxy, cosmic rays (CRs) are expected to exist in the space between galaxies. Shocks wa...
Shock waves emerge following the rapid release of energy in a flow. The interaction of shocks with i...
Cosmological shock waves are tracers of the thermal history of the structures in the Universe. They ...
Explosive astrophysical phenomena have historically played a significant role in understanding the u...
Supersonic flows are expected to exist in the atmospheres of irradiated exoplanets, but the question...
International audienceContemporary lasers allow us to create shocks in the laboratory that propagate...
Cosmological shock waves are ubiquitous to cosmic structure formation and evolution. As a consequenc...
Why do we study shocks ? Because they are there. Shocks are ubiquitous in the interstellar medium (I...
Supernovae launch spherical shocks into the circumstellar medium (CSM). These shocks may interact wi...
We study the properties of cosmological shock waves identified in high-resolution, N-body/hydrodynam...
Understanding the causes and effects of explosions is important to experts in a broad range of disci...
Shock waves form in the intergalactic medium (IGM) as a consequence of accretion, merger, and turbul...
Cosmological shock waves are induced during hierarchical formation of large-scale structure in the u...
Bubbles in the interstellar medium are produced by astrophysical sources, which continuously or expl...
Star formation in general, and starbursts in particular, drive the evolution of galaxies. To underst...
Like in our galaxy, cosmic rays (CRs) are expected to exist in the space between galaxies. Shocks wa...
Shock waves emerge following the rapid release of energy in a flow. The interaction of shocks with i...
Cosmological shock waves are tracers of the thermal history of the structures in the Universe. They ...
Explosive astrophysical phenomena have historically played a significant role in understanding the u...
Supersonic flows are expected to exist in the atmospheres of irradiated exoplanets, but the question...
International audienceContemporary lasers allow us to create shocks in the laboratory that propagate...
Cosmological shock waves are ubiquitous to cosmic structure formation and evolution. As a consequenc...
Why do we study shocks ? Because they are there. Shocks are ubiquitous in the interstellar medium (I...
Supernovae launch spherical shocks into the circumstellar medium (CSM). These shocks may interact wi...
We study the properties of cosmological shock waves identified in high-resolution, N-body/hydrodynam...
Understanding the causes and effects of explosions is important to experts in a broad range of disci...