Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Di Mascia, F."'
Autor:
Markov, V., Gallerani, S., Ferrara, A., Pallottini, A., Parlanti, E., Di Mascia, F., Sommovigo, L., Kohandel, M.
A sizable fraction of the heavy elements synthesized by stars in galaxies condenses into sub-micron-sized solid-state particles, known as dust grains. Dust produces a wavelength-dependent attenuation, $A_\lambda$, of the galaxy emission, thereby sign
Externí odkaz:
http://arxiv.org/abs/2402.05996
Autor:
Tripodi, R., Feruglio, C., Fiore, F., Zappacosta, L., Piconcelli, E., Bischetti, M., Bongiorno, A., Carniani, S., Civano, F., Chen, C. -C., Cristiani, S., Cupani, G., Di Mascia, F., D'Odorico, V., Fan, X., Ferrara, A., Gallerani, S., Ginolfi, M., Maiolino, R., Mainieri, V., Marconi, A., Saccheo, I., Salvestrini, F., Tortosa, A., Valiante, R.
We used low- to high-frequency ALMA observations to investigate the cold gas and dust in ten QSOs at $z\gtrsim 6$. Our analysis of the CO(6-5) and CO(7-6) emission lines in the selected QSOs provided insights into their molecular gas masses, which av
Externí odkaz:
http://arxiv.org/abs/2401.04211
Autor:
Markov, V., Gallerani, S., Pallottini, A., Sommovigo, L., Carniani, S., Ferrara, A., Parlanti, E., Di Mascia, F.
Publikováno v:
A&A 679, A12 (2023)
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:
http://arxiv.org/abs/2304.11178
Autor:
Pallottini, A., Ferrara, A., Gallerani, S., Behrens, C., Kohandel, M., Carniani, S., Vallini, L., Salvadori, S., Gelli, V., Sommovigo, L., D'Odorico, V., Di Mascia, F., Pizzati, E.
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:
http://arxiv.org/abs/2201.02636
Autor:
Di Mascia, F., Gallerani, S., Ferrara, A., Pallottini, A., Maiolino, R., Carniani, S., D'Odorico, V.
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:
http://arxiv.org/abs/2106.15625
Autor:
Di Mascia, F., Gallerani, S., Behrens, C., Pallottini, A., Carniani, S., Ferrara, A., Barai, P., Vito, F., Zana, T.
We investigate the infrared (IR) emission of high-redshift ($z\sim 6$), highly star-forming (${ {\rm SFR} > 100}$ $M_{\rm \odot} {\rm yr}^{-1}$) galaxies, with/without Active Galactic Nuclei (AGN), using a suite of cosmological simulations featuring
Externí odkaz:
http://arxiv.org/abs/2102.08956