Zobrazeno 1 - 10
of 16 048
pro vyhledávání: '"Facchini, A"'
Autor:
Maucó, K., Manara, C. F., Bayo, A., Hernández, J., Campbell-White, J., Calvet, N., Ballabio, G., Aru, M. L., Alcalá, J. M., Ansdell, M., Briceño, C., Facchini, S., Haworth, T. J., McClure, M., Williams, J. P.
Disk winds play a crucial role in the evolution of protoplanetary disks. Typical conditions for star and planet formation are in regions with intermediate or strong UV radiation fields produced by massive stars. The $\sigma$-Orionis cluster is the id
Externí odkaz:
http://arxiv.org/abs/2411.19741
Autor:
Aru, Mari-Liis, Mauco, Karina, Manara, Carlo F., Haworth, Thomas J., Ballering, Nick, Boyden, Ryan, Campbell-White, Justyn, Facchini, Stefano, Rosotti, Giovanni P., Winter, Andrew, Miotello, Anna, McLeod, Anna F., Robberto, Massimo, Petr-Gotzens, Monika G., Ballabio, Giulia, Vicente, Silvia, Ansdell, Megan, Cleeves, L. Ilsedore
The evolution of protoplanetary disks in regions with massive OB stars is influenced by externally driven winds that deplete the outer parts of disks. These winds have previously been studied via forbidden oxygen emission lines, which also arise in i
Externí odkaz:
http://arxiv.org/abs/2410.21018
Phyllotactic patterns, i.e. regular arrangements of leaves or seeds around a plant stem, are fascinating examples of complex structures encountered in Nature. In botany, their symmetries develop when a new primordium periodically grows in the largest
Externí odkaz:
http://arxiv.org/abs/2410.01596
In recent years, the dissemination of machine learning (ML) methodologies in scientific research has prompted discussions on theory ladenness. More specifically, the issue of theory ladenness has remerged as questions about whether and how ML models
Externí odkaz:
http://arxiv.org/abs/2409.11277
Autor:
Kurtovic, N. T., Facchini, S., Benisty, M., Pinilla, P., Cabrit, S., Jensen, E. L. N., Dougados, C., Booth, R., Kimmig, C. N., Manara, C. F., Rodriguez, J. E.
The dynamical interactions between young binaries can perturb the material distribution of their circumstellar disks, and modify the planet formation process. In order to constrain the impact and nature of the binary interaction in the RW Aur system
Externí odkaz:
http://arxiv.org/abs/2407.18828
Autor:
Rampinelli, L., Facchini, S., Leemker, M., Bae, J., Benisty, M., Teague, R., Law, C. J., Öberg, K. I., Portilla-Revelo, B., Cridland, A. J.
Publikováno v:
A&A 689, A65 (2024)
With two directly detected protoplanets, the PDS 70 system is a unique source in which to study the complex interplay between forming planets and their natal environment. The large dust cavity carved by the two giant planets can affect the disk chemi
Externí odkaz:
http://arxiv.org/abs/2407.06272
Autor:
Veronesi, Benedetta, Longarini, Cristiano, Lodato, Giuseppe, Laibe, Guillaume, Hall, Cassandra, Facchini, Stefano, Testi, Leonardo
Publikováno v:
A&A 688, A136 (2024)
The mass of protoplanetary discs sets the amount of material available for planet formation, determines the level of coupling between gas and dust, and possibly sets gravitational instabilities. Measuring mass of discs is challenging, since it is not
Externí odkaz:
http://arxiv.org/abs/2405.15944
Autor:
Rubegni, Elisa, Ayoub, Omran, Rizzo, Stefania Maria Rita, Barbero, Marco, Bernegger, Guenda, Faraci, Francesca, Mangili, Francesca, Soldini, Emiliano, Trimboli, Pierpaolo, Facchini, Alessandro
The widespread use of Artificial Intelligence-based tools in the healthcare sector raises many ethical and legal problems, one of the main reasons being their black-box nature and therefore the seemingly opacity and inscrutability of their characteri
Externí odkaz:
http://arxiv.org/abs/2404.04638
Human-centered explainable AI (HCXAI) advocates for the integration of social aspects into AI explanations. Central to the HCXAI discourse is the Social Transparency (ST) framework, which aims to make the socio-organizational context of AI systems ac
Externí odkaz:
http://arxiv.org/abs/2403.17873
Autor:
Aru, Mari-Liis, Mauco, Karina, Manara, Carlo F., Haworth, Thomas J., Facchini, Stefano, McLeod, Anna F., Miotello, Anna, Petr-Gotzens, Monika G., Robberto, Massimo, Rosotti, Giovanni P., Vicente, Silvia, Winter, Andrew, Ansdell, Megan
Publikováno v:
A&A 687, A93 (2024)
In the Orion Nebula Cluster (ONC), protoplanetary disks exhibit ionized gas clouds in the form of a striking teardrop shape as massive stars irradiate the disk material. We present the first spatially and spectrally resolved observations of 12 proply
Externí odkaz:
http://arxiv.org/abs/2403.12604