Zobrazeno 1 - 10
of 7 459
pro vyhledávání: '"López, I."'
Autor:
Sengupta, D., Torres-Albà, N., Pizzetti, A., López, I. E., Marchesi, S., Vignali, C., Barchiesi, L., Cox, I., Gaspari, M., Zhao, X., Ajello, M., Esposito, F.
Most of the super-massive black holes in the Universe accrete material in an obscured phase. While it is commonly accepted that the "dusty torus" is responsible for the nuclear obscuration, its geometrical, physical, and chemical properties are far f
Externí odkaz:
http://arxiv.org/abs/2410.02878
Autor:
López-López, X., Bolzonella, M., Pozzetti, L., Salvato, M., Bisigello, L., Feltre, A., López, I. E., Viitanen, A., Allevato, V., Bongiorno, A., Girelli, G., Buchner, J., Charlot, S., Ricci, F., Schreiber, C., Zamorani, G.
Publikováno v:
A&A 691, A136 (2024)
Aims. We present MAMBO, a flexible and efficient workflow to build empirical galaxy and Active Galactic Nuclei (AGN) mock catalogues that reproduce the physical and observational properties of these sources. Methods. We start from simulated dark matt
Externí odkaz:
http://arxiv.org/abs/2409.06700
Autor:
Bertola, E., Circosta, C., Ginolfi, M., Mainieri, V., Vignali, C., Rivera, G. Calistro, Ward, S. R., Lopez, I. E., Pensabene, A., Alexander, D. M., Bischetti, M., Brusa, M., Cappi, M., Comastri, A., Contursi, A., Cicone, C., Cresci, G., Dadina, M., D'Amato, Q., Feltre, A., Harrison, C. M., Kakkad, D., Lamperti, I., Lanzuisi, G., Mannucci, F., Marconi, A., Perna, M., Piconcelli, E., Puglisi, A., Ricci, F., Scholtz, J., Tozzi, G., Vietri, G., Zamorani, G., Zappacosta, L.
The energy released by AGN has the potential to heat or remove the gas of the ISM, thus likely impacting the cold molecular gas reservoir of host galaxies at first, with star formation following on longer timescales. Previous works on high-z galaxies
Externí odkaz:
http://arxiv.org/abs/2408.16821
Autor:
López, I. E., Yang, G., Mountrichas, G., Brusa, M., Alexander, D. M., Baldi, R. D., Bertola, E., Bonoli, S., Comastri, A., Shankar, F., Acharya, N., Tetilla, A. V. Alonso, Lapi, A., Laloux, B., López, X. López, Rodríguez, I. Muñoz, Musiimenta, B., Clavijo, N. Osorio, Sala, L., Sengupta, D.
The spectral energy distribution (SED) of low-luminosity active galactic nuclei (LLAGN) presents unique challenges due to their comparable radiation output to their host galaxies and complex accretion dynamics. We introduce a novel module within the
Externí odkaz:
http://arxiv.org/abs/2404.16938
Autor:
Baldini, P., Lanzuisi, G., Brusa, M., Merloni, A., Gkimisi, K., Perna, M., Lopez, I. E., Bertola, E., Igo, Z., Waddell, S., Musiimenta, B., Aydar, C., Arcodia, R., Matzeu, G. A., Luminari, A., Buchner, J., Vignali, C., Dadina, M., Comastri, A., Cresci, G., Marchesi, S., Gilli, R., Tombesi, F., Serafinelli, R.
Publikováno v:
A&A 686, A217 (2024)
Powerful outflows from active galactic nuclei (AGN) can significantly impact the gas reservoirs of their host galaxies. However, it is still unclear how these outflows can propagate from the very central regions of galaxies to their outskirts, and wh
Externí odkaz:
http://arxiv.org/abs/2402.16966
Autor:
Garate-Lopez, I., Lebonnois, Sébastien
Publikováno v:
Icarus, vol. 314, 1-11 (2018)
Global Climate Models (GCM) are very useful tools to study theoretically the general dynamics and specific phenomena in planetary atmospheres. In the case of Venus, several GCMs succeeded in reproducing the atmosphere's superrotation and the global t
Externí odkaz:
http://arxiv.org/abs/2402.04057
Publikováno v:
Planetary and Space Science, vol. 81, 65-73 (2013)
Thermal radiation becomes a prominent feature in the continuum spectrum of Venus longwards of $\sim$3 $\mu$m. The emission is traceable to the upper cloud and haze layers in the planet's mesosphere. Venus' thermal radiation spectrum is punctuated by
Externí odkaz:
http://arxiv.org/abs/2402.03926
Publikováno v:
Journal of Geophysical Research: Planets, vol. 121, 574-593 (2016)
Venus' atmosphere shows highly variable warm vortices over both of the planet's poles. The nature of the mechanism behind their formation and properties is still unknown. Potential vorticity is a conserved quantity when advective processes dominate o
Externí odkaz:
http://arxiv.org/abs/2402.00679
Publikováno v:
Icarus, vol. 245, 16-31 (2015)
The Venus thermal radiation spectrum exhibits the signature of $CO_2$ absorption bands. By means of inversion techniques, those bands enable the retrieval of atmospheric temperature profiles. We have analyzed VIRTIS-M-IR night-side data obtaining hig
Externí odkaz:
http://arxiv.org/abs/2401.17946
Autor:
Sánchez-Lavega, A., García-Melendo, E., Perez-Hoyos, S., Hueso, R., Wong, M. H., Simon, A., Sanz-Requena, J. F., Antuñano, A., Barrado-Izagirre, N., Garate-Lopez, I., Rojas, J. F., Gaztelurrutia, T. del Rio, Gómez-Forrellad, J. M., de Pater, I., Li, L., Barry, T., contributors, PVOL
Publikováno v:
Nature Communications, vol. 7, article number: 13626 (2016)
Saturn has an intense and broad eastward equatorial jet with a complex three-dimensional structure mixed with time variability. The equatorial region experiences strong seasonal insolation variations enhanced by ring shadowing and three of the six kn
Externí odkaz:
http://arxiv.org/abs/2401.17833