Zobrazeno 1 - 10
of 1 881
pro vyhledávání: '"D'Elía, G."'
Hot Jupiters (HJs) are giant planets with orbital periods of the order of a few days with semimajor axis within $\sim$0.1 au. Several theories have been invoked in order to explain the origin of this type of planets, one of them being the high-eccent
Externí odkaz:
http://arxiv.org/abs/2210.11760
Publikováno v:
A&A 639, A9 (2020)
Aims. We developed a six-part collisional evolution model of the main asteroid belt (MB) and used it to study the contribution of the different regions of the MB to the near-earth asteroids (NEAs). Methods. We built a statistical code called ACDC tha
Externí odkaz:
http://arxiv.org/abs/2005.12858
Akademický článek
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Autor:
Ronco, M. P., de Elía, G. C.
This work is the second part of a project that attempts to analyze the formation of Solar system analogues (SSAs) from the gaseous to the post-gas phase, in a self-consistently way. In the first paper (PI) we presented our model of planet formation d
Externí odkaz:
http://arxiv.org/abs/1807.01429
Autor:
Nolasco, Mary C., Flores, Lucia F., Gutiérrez, Emmanuel J., Aguilar, Javier, Palacios, Elia G., Flores, Mizraim U., Rodríguez, Israel, Reyes, Iván A.
Publikováno v:
In Hydrometallurgy June 2022 212
Autor:
Dinardo, F.R., Maggiolino, A. *, Martinello, T., Liuzzi, G.M., Elia, G., Zizzo, N., Latronico, T., Mastrangelo, F., Dahl, G.E., De Palo, P.
Publikováno v:
In Journal of Dairy Science May 2022 105(5):4393-4409
Publikováno v:
A&A 607, A63 (2017)
Several observational works have shown the existence of Jupiter-mass planets covering a wide range of semi-major axes around Sun-like stars. We aim to analyse the planetary formation processes around Sun-like stars that host a Jupiter-mass planet at
Externí odkaz:
http://arxiv.org/abs/1708.00290
Population synthesis models of planetary systems developed during the last $\sim$15 years could reproduce several of the observables of the exoplanet population, and also allowed to constrain planetary formation models. We present our planet formatio
Externí odkaz:
http://arxiv.org/abs/1705.08608
Publikováno v:
A&A 605, A64 (2017)
We analyze the process of planetary scattering around M0-type stars. To do this, we carry out N-body simulations with three Jupiter-mass planets close to their instability limit together with an outer planetesimal disk. This paper focuses on the anal
Externí odkaz:
http://arxiv.org/abs/1701.03865
Akademický článek
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