Zobrazeno 1 - 5
of 5
pro vyhledávání: '"K. J. A. Goldsmith"'
Autor:
Julian M. Pittard, K. J. A. Goldsmith
Studies of filamentary structures that are prevalent throughout the interstellar medium are of great significance to a number of astrophysical fields. Here, we present 3D hydrodynamic simulations of shock-filament interactions where the equation of s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a7499d8ccc5637baff3957a5846a4f5c
Autor:
Julian M. Pittard, K. J. A. Goldsmith
The similarities, or otherwise, of a shock or wind interacting with a cloud of density contras t$ \chi = 10$ were explored in a previous paper. Here, we investigate such interactions with clouds of higher density contrast. We compare the adiabatic hy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::33d60ce381a1d8b5845d9e3b0109e3aa
http://arxiv.org/abs/1805.04709
http://arxiv.org/abs/1805.04709
Autor:
K. J. A. Goldsmith, Julian M. Pittard
The interaction of a hot, high-velocity wind with a cold, dense molecular cloud has often been assumed to resemble the evolution of a cloud embedded in a post-shock flow. However, no direct comparative study of these two processes currently exists in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c54c8cb20a7ae1be4bf480f0317bafae
Autor:
Julian M. Pittard, K. J. A. Goldsmith
We present 3D magnetohydrodynamic numerical simulations of the adiabatic interaction of a shock with a dense, filamentary cloud. We investigate the effects of various filament lengths and orientations on the interaction using different orientations o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d4ba9c0b7f68456177dba4cf7fe2356
http://arxiv.org/abs/1607.03929
http://arxiv.org/abs/1607.03929
Autor:
K. J. A. Goldsmith, Julian M. Pittard
We present 3D hydrodynamic adiabatic simulations of a shock interacting with a dense, elongated cloud. We compare how the nature of the interaction changes with the filament's length and its orientation to the shock, and with the shock Mach number an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef6f0fa6e4754cab234f1d5e282a82c9
http://arxiv.org/abs/1512.06041
http://arxiv.org/abs/1512.06041