Zobrazeno 1 - 10
of 206
pro vyhledávání: '"Mingozzi, M"'
Autor:
Huberty, M., Carr, C., Scarlata, C., Heckman, T., Henry, A., Xu, X., Arellano-Córdoba, K., Berg, D., Charlot, S., Chisholm, J., Gazagnes, S., Hayes, M., Hu, W., James, B., Jennings, R. M., Leitherer, C., Martin, C. L., Mingozzi, M., Skillman, E., Sugahara, Y.
Feedback driven massive outflows play a crucial role in galaxy evolution by regulating star formation and influencing the dynamics of surrounding media. Extracting outflow properties from spectral lines is a notoriously difficult process for a number
Externí odkaz:
http://arxiv.org/abs/2406.03646
Autor:
Ulivi, L., Venturi, G., Cresci, G., Marconi, A., Marconcini, C., Amiri, A., Belfiore, F., Bertola, E., Carniani, S., Amato, Q. D, Di Teodoro, E., Ginolfi, M., Girdhar, A., Harrison, C., Maiolino, R., Mannucci, F., Mingozzi, M., Perna, M., Scialpi, M., Tomicic, N., Tozzi, G., Treister, E.
Publikováno v:
A&A 685, A122 (2024)
An increasing number of observations and simulations suggests that low-power (<10$^{44}$ erg s$^{-1}$) jets may be a significant channel of feedback produced by active galactic nuclei (AGN), but little is known about their actual effect on their host
Externí odkaz:
http://arxiv.org/abs/2403.01258
Autor:
Marconi, A., Amiri, A., Feltre, A., Belfiore, F., Cresci, G., Curti, M., Mannucci, F., Bertola, E., Brazzini, M., Carniani, S., Cataldi, E., D'Amato, Q., de Rosa, G., Di Teodoro, E., Ginolfi, M., Kumari, N., Marconcini, C., Maiolino, R., Magrini, L., Marasco, A., Mingozzi, M., Moreschini, B., Nagao, T., Oliva, E., Scialpi, M., Tomicic, N., Tozzi, G., Ulivi, L., Venturi, G.
Publikováno v:
A&A 689, A78 (2024)
We present HOMERUN (Highly Optimized Multi-cloud Emission-line Ratios Using photo-ionizatioN), a new approach to modelling emission lines from photoionized gas that can simultaneously reproduce all observed line intensities from a wide range of ioniz
Externí odkaz:
http://arxiv.org/abs/2401.13028
MOKA3D: An innovative approach to 3D gas kinematic modelling. I. Application to AGN ionized outflows
Autor:
Marconcini, C., Marconi, A., Cresci, G., Venturi, G., Ulivi, L., Mannucci, F., Belfiore, F., Tozzi, G., Ginolfi, M., Marasco, A., Carniani, S., Amiri, A., Di Teodoro, E., Scialpi, M., Tomicic, N., Mingozzi, M., Brazzini, M., Moreschini, B.
Publikováno v:
A&A 677, A58 (2023)
Studying the feedback process of Active Galactic Nuclei (AGN) requires characterising multiple kinematical components, such as rotating gas and stellar disks, outflows, inflows, and jets. To compare the observed properties with theoretical prediction
Externí odkaz:
http://arxiv.org/abs/2307.01854
Autor:
Bacchini, C., Mingozzi, M., Poggianti, B. M., Moretti, A., Gullieuszik, M., Marasco, A., Sodi, B. Cervantes, Sánchez-García, O., Vulcani, B., Werle, A., Paladino, R., Radovich, M.
Cluster galaxies are subject to the ram pressure exerted by the intracluster medium, which can perturb or even strip away their gas while leaving the stars undisturbed. We model the distribution and kinematics of the stars and the molecular gas in fo
Externí odkaz:
http://arxiv.org/abs/2301.03090
Autor:
Marasco, A., Belfiore, F., Cresci, G., Lelli, F., Venturi, G., Hunt, L. K., Concas, A., Marconi, A., Mannucci, F., Mingozzi, M., McLeod, A. F., Kumari, N., Carniani, S., Vanzi, L., Ginolfi, M.
Publikováno v:
A&A 670, A92 (2023)
Baryonic feedback is expected to play a key role in regulating the star formation of low-mass galaxies by producing galaxy-scale winds associated with mass-loading factors $\beta\!\sim\!1\!-\!50$. We have tested this prediction using a sample of 19 n
Externí odkaz:
http://arxiv.org/abs/2209.02726
Autor:
Mannucci, F., Belfiore, F., Curti, M., Cresci, G., Maiolino, R., Marasco, A., Marconi, A., Mingozzi, M., Tozzi, G., Amiri, A.
The Diffuse Ionized Gas (DIG) contributes to the nebular emission of galaxies, resulting in emission line flux ratios that can be significantly different from those produced by HII regions. Comparing the emission of [SII]6717,31 between pointed obser
Externí odkaz:
http://arxiv.org/abs/2109.02684
Autor:
Vulcani, B., Poggianti, B. M., Moretti, A., Franchetto, A., Bacchini, C., McGee, S., Jaffe, Y. L., Mingozzi, M., Werle, A., Tomicic, N., Fritz, J., Bettoni, D., Wolter, A., Gullieuszik, M.
Galaxies inhabit a wide range of environments and therefore are affected by different physical mechanisms. Spatially resolved maps combined with the knowledge of the hosting environment are very powerful to classify galaxies by physical process. In t
Externí odkaz:
http://arxiv.org/abs/2104.02089
Autor:
Tozzi, G., Cresci, G., Marasco, A., Nardini, E., Marconi, A., Mannucci, F., Chartas, G., Rizzo, F., Amiri, A., Brusa, M., Comastri, A., Dadina, M., Lanzuisi, G., Mainieri, V., Mingozzi, M., Perna, M., Venturi, G., Vignali, C.
Publikováno v:
A&A 648, A99 (2021)
Outflows driven by active galactic nuclei (AGN) are expected to have a significant impact on the host galaxy evolution, but it is still debated how they are accelerated and propagate on galaxy-wide scales. This work addresses these questions by study
Externí odkaz:
http://arxiv.org/abs/2102.07789
Autor:
Venturi, G., Cresci, G., Marconi, A., Mingozzi, M., Nardini, E., Carniani, S., Mannucci, F., Marasco, A., Maiolino, R., Perna, M., Treister, E., Bland-Hawthorn, J., Gallimore, J.
Outflows accelerated by AGN are commonly observed in the form of coherent, mildly collimated high-velocity gas directed along the AGN ionisation cones and kinetically powerful (>$10^{44-45}$ erg/s) jets. Recent works found that outflows can also be a
Externí odkaz:
http://arxiv.org/abs/2011.04677