Zobrazeno 1 - 10
of 8 935
pro vyhledávání: '"A. Manara"'
Autor:
Acclavio, Matteo, Manara, Giulia
In this paper, we establish the foundations of a novel logical framework for the {\pi}-calculus, based on the deduction-as-computation paradigm. Following the standard proof-theoretic interpretation of logic programming, we represent processes as for
Externí odkaz:
http://arxiv.org/abs/2411.08847
Autor:
Donati, J. -F., Cristofari, P. I., Alencar, S. H. P., Kóspál, Á., Bouvier, J., Moutou, C., Carmona, A., Gregorio-Hetem, J., Manara, C. F., Artigau, E., Doyon, R., Takami, M., Shang, H., Nascimento, J. Dias do, Ménard, F., Gaidos, E., team, the SPIRou science
This paper presents near-infrared spectropolarimetric and velocimetric observations of the young planet-hosting T Tauri star PDS 70, collected with SPIRou at the 3.6m Canada-France-Hawaii Telescope from 2020 to 2024. Clear Zeeman signatures from magn
Externí odkaz:
http://arxiv.org/abs/2411.03089
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
Autor:
Micolta, Marbely, Calvet, Nuria, Thanathibodee, Thanawuth, C., Gladis Magris, Manara, Carlo F., Venuti, Laura, Alcalá, Juan Manuel, Herczeg, Gregory J.
We present a study of the abundance of calcium in the innermost disk of 70 T Tauri stars in the star-forming regions of Chamaeleon I, Lupus and Orion OB1b. We use calcium as a proxy for the refractory material that reaches the inner disk. We used mag
Externí odkaz:
http://arxiv.org/abs/2410.17327
Publikováno v:
A&A 691, A169 (2024)
Growing evidence suggests that protoplanetary discs may be influenced by late stage infall from the interstellar medium (ISM). It remains unclear the degree to which infall shapes disc populations at ages $\gtrsim 1$~Myr. We explore possible spatial
Externí odkaz:
http://arxiv.org/abs/2409.17220
Autor:
De Furio, Matthew, Meyer, Michael R., Greene, Thomas, Hodapp, Klaus, Johnstone, Doug, Leisenring, Jarron, Rieke, Marcia, Robberto, Massimo, Roellig, Thomas, Cugno, Gabriele, Fiorellino, Eleonora, Manara, Carlo, Raileanu, Roberta, van Terwisga, Sierk
A successful theory of star formation should predict the number of objects as a function of their mass produced through star-forming events. Previous studies in star-forming regions and the solar neighborhood identify a mass function increasing from
Externí odkaz:
http://arxiv.org/abs/2409.04624
Autor:
Armeni, A., Stelzer, B., Frasca, A., Manara, C. F., Walter, F. M., Alcalá, J. M., Schneider, P. C., Sicilia-Aguilar, A., Campbell-White, J., Fiorellino, E., Gameiro, J. F., Gangi, M.
The aim of this work is to characterize the accretion process of the classical T Tauri Star RU Lup. We studied optical high-resolution spectroscopic observations from CHIRON and ESPRESSO, obtained simultaneously with photometric data from AAVSO and T
Externí odkaz:
http://arxiv.org/abs/2408.14996
Autor:
Zaire, B., Donati, J. -F., Alencar, S. P., Bouvier, J., Moutou, C., Bellotti, S., Carmona, A., Petit, P., Kóspál, Á., Shang, H., Grankin, K., Manara, C., Alecian, E., Gregory, S. P., Fouqué, P., consortium, the SLS
This paper analyses spectropolarimetric observations of the classical T Tauri star (CTTS) GM Aurigae collected with SPIRou, the near-infrared spectropolarimeter at the Canada-France-Hawaii Telescope, as part of the SLS and SPICE Large Programs. We re
Externí odkaz:
http://arxiv.org/abs/2408.05864
Autor:
Wendeborn, John, Espaillat, Catherine C., Thanathibodee, Thanawuth, Robinson, Connor E., Pittman, Caeley V., Calvet, Nuria, Muzerolle, James, Walter, Fredrick M., Eisloffel, Jochen, Fiorellino, Eleonora, Manara, Carlo F., Kospal, Agnes, Abraham, Peter, Claes, Rik, Rigliaco, Elisabetta, Venuti, Laura, Campbell-White, Justyn, McGinnis, Pauline, Gangi, Manuele, Mauco, Karina, Gameiro, Filipe, Frasca, Antonio, Guo, Zhen
Classical T Tauri Stars (CTTSs) are highly variable stars that possess gas- and dust-rich disks from which planets form. Much of their variability is driven by mass accretion from the surrounding disk, a process that is still not entirely understood.
Externí odkaz:
http://arxiv.org/abs/2408.04465
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