Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Di Mascia, F."'
Autor:
Markov, V., Gallerani, S., Pallottini, A., Sommovigo, L., Carniani, S., Ferrara, A., Parlanti, E., Di Mascia, F.
Attenuation curves in galaxies depend on dust chemical composition, content, and grain size distribution. Such parameters are related to intrinsic galaxy properties such as metallicity, star formation rate, and stellar age. Due to the lack of observa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ad1e63e5e1f13934f4ed640ae69d89f5
http://arxiv.org/abs/2304.11178
http://arxiv.org/abs/2304.11178
Autor:
A Pallottini, A Ferrara, S Gallerani, C Behrens, M Kohandel, S Carniani, L Vallini, S Salvadori, V Gelli, L Sommovigo, V D’Odorico, F Di Mascia, E Pizzati
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 513(4), 5621-5641
We introduce SERRA, a suite of zoom-in high-resolution ($\sim 10\,\rm pc$) cosmological simulations including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post-processed to derive galaxy UV+FIR continuum and emission l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::22149e65baadbbcc6ebe3841012f4e92
https://hdl.handle.net/11384/126388
https://hdl.handle.net/11384/126388
Autor:
Simona Gallerani, S. Carniani, Roberto Maiolino, Valentina D'Odorico, Andrea Pallottini, F. Di Mascia, Andrea Ferrara
We investigate the attenuation law in $z\sim 6$ quasars by combining cosmological zoom-in hydrodynamical simulations of quasar host galaxies, with multi-frequency radiative transfer calculations. We consider several dust models differing in terms of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5b00744cb5b7bbfb9a2f1f9208944ec
http://arxiv.org/abs/2106.15625
http://arxiv.org/abs/2106.15625