Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Martin Glatzle"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 510:1068-1082
The presence of charged dust grains is known to have a profound impact on the physical evolution of the multiphase interstellar medium (ISM). Despite its importance, this process is still poorly explored in numerical simulations due to its complex ph
Autor:
Annalisa Pillepich, Lars Hernquist, Mark Vogelsberger, Chris Byrohl, Dylan Nelson, Martin Glatzle, Christoph Behrens, Federico Marinacci, Ivan Kostyuk
Extended Lyman-alpha emission is now commonly detected around high redshift galaxies through stacking and even on individual basis. Despite recent observational advances, the physical origin of these Lyman-alpha halos (LAHs), as well as their relatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f1a2b03ba0f14cdfd8195d61c070d7c1
http://arxiv.org/abs/2009.07283
http://arxiv.org/abs/2009.07283
Autor:
L. K. Hunt, Martin Glatzle, L. Graziani, Raffaella Schneider, U. Maio, Michele Ginolfi, B. Ciardi
The recent discovery of high redshift dusty galaxies implies a rapid dust enrichment of their interstellar medium (ISM). To interpret these observations, we run a cosmological simulation in a 30$h^{-1}$ cMpc/size volume down to $z \approx 4$. We use
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47cd86e9b9a6236f6e14198c94c38068
We present a new dust extension to the Monte Carlo radiative transfer code crash, which enables it to simulate the propagation of ionizing radiation through mixtures of gas and dust. The new code is applied to study the impact of dust absorption on i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::65677df447ffa3698809318375aea55c
http://arxiv.org/abs/1809.04132
http://arxiv.org/abs/1809.04132
Publikováno v:
arXiv.org e-Print Archive
We investigate the impact of quasars on the ionization of the surrounding intergalactic medium (IGM) with the radiative transfer code \texttt{CRASH4}, now accounting for X-rays and secondary electrons. After comparing with analytic solutions, we post
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f9d0fb8eb675e757ea3548f9a19fdb9