Zobrazeno 1 - 10
of 16 082
pro vyhledávání: '"A. FACCHINI"'
Autor:
Xie, Chen, Xie, Chengyan, Ren, Bin B., Benisty, Myriam, Ginski, Christian, Fang, Taotao, Casassus, Simon, Bae, Jaehan, Facchini, Stefano, Ménard, François, van Holstein, Rob G.
In the early stages of planetary system formation, young exoplanets gravitationally interact with their surrounding environments and leave observable signatures on protoplanetary disks. Among these structures, a pair of nearly symmetric spiral arms c
Externí odkaz:
http://arxiv.org/abs/2412.14402
Autor:
Calò, Emanuele, Facchini, Angelo
In Regional Economics, the attractiveness of regions for capital, migrants, tourists, and other kinds of flows is a relevant topic. Usually, studies in this field have mainly explored single flows, characterizing the dimensions of territorial attract
Externí odkaz:
http://arxiv.org/abs/2412.09178
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
Publikováno v:
World Cancer Research Journal, Vol 9 (2022)
Objective: Health care accounts for up to 8-10% of greenhouse emission yearly in the US and surgical room contributes an estimated 25-30% of hospital waste. Despite the major role of greenhouse emissions because of surgery, little has been done by su
Externí odkaz:
https://doaj.org/article/63eeb3f1a92d45e6a0bc6edb317c0d5c
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
Publikováno v:
A&A 692, A137 (2024)
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