Zobrazeno 1 - 10
of 53
pro vyhledávání: '"Sucerquia, Mario"'
Autor:
Sucerquia, Mario, Alvarado-Montes, Jaime A., Zuluaga, Jorge I., Cuello, Nicolás, Cuadra, Jorge, Montesinos, Matías
Rings are complex structures surrounding giant planets and some minor bodies in the Solar System. While some formation mechanisms could also potentially foster their existence around (regular or irregular) satellites, none of these bodies currently b
Externí odkaz:
http://arxiv.org/abs/2408.10643
Autor:
Veenstra, Allard K., Zuluaga, Jorge I., Alvarado-Montes, Jaime A., Sucerquia, Mario, Stam, Daphne M.
We explore the potential of polarimetry as a tool for detecting and characterizing exorings. For that purpose, we have improved the publicly available photometric code Pryngles by adding the results of radiative transfer calculations that fully inclu
Externí odkaz:
http://arxiv.org/abs/2404.16606
Autor:
Cuello, Nicolás, Sucerquia, Mario
Alpha Centauri is a triple stellar system, and it contains the closest star to Earth (Proxima Centauri). Over the last decades, the stars in Alpha Cen and their orbits have been investigated in great detail. However, the possible scenarios for planet
Externí odkaz:
http://arxiv.org/abs/2401.16003
Publikováno v:
Astronomy and Computing 40 (2022) 100623
Rings around exoplanets (exorings) are one of the most expected discoveries in exoplanetary research. There is an increasing number of theoretical and observational efforts for detecting exorings, but none of them have succeeded yet. Most of those me
Externí odkaz:
http://arxiv.org/abs/2207.08636
Autor:
Sucerquia, Mario, Alvarado-Montes, Jaime A., Bayo, Amelia, Cuadra, Jorge, Cuello, Nicolás, Giuppone, Cristian A., Montesinos, Matías, Olofsson, J., Schwab, Christian, Spitler, Lee, Zuluaga, Jorge I.
In recent years, technical and theoretical work to detect moons and rings around exoplanets has been attempted. The small mass/size ratios between moons and planets means this is very challenging, having only one exoplanetary system where spotting an
Externí odkaz:
http://arxiv.org/abs/2112.02687
Autor:
Alvarado-Montes, Jaime A., Sucerquia, Mario, García-Carmona, Carolina, Zuluaga, Jorge I., Spitler, Lee, Schwab, Christian
Unveiling the fate of ultra-short period (USP) planets may help us understand the qualitative agreement between tidal theory and the observed exoplanet distribution. Nevertheless, due to the time-varying interchange of spin-orbit angular momentum in
Externí odkaz:
http://arxiv.org/abs/2104.05967
Autor:
Montesinos, Matias, Garrido-Deutelmoser, Juan, Olofsson, Johan, Giuppone, Cristian A., Cuadra, Jorge, Bayo, Amelia, Sucerquia, Mario, Cuello, Nicolas
Publikováno v:
A&A 642, A224 (2020)
Trojans are defined as objects that share the orbit of a planet at the stable Lagrangian points $L_4$ and $L_5$. In the Solar System, these bodies show a broad size distribution ranging from micrometer($\mu$m) to centimeter(cm) particles (Trojan dust
Externí odkaz:
http://arxiv.org/abs/2009.10768
Autor:
Sucerquia, Mario, Alvarado-Montes, Jaime A., Zuluaga, Jorge I., Montesinos, Matías, Bayo, Amelia
Rings around giant exoplanets (hereafter 'exorings') are still a missing planetary phenomenon among the vast number of discovered planets. Despite the fact there exist a large number of methods for identifying and characterizing these exorings, none
Externí odkaz:
http://arxiv.org/abs/2004.14121
Exoplanet discoveries have motivated numerous efforts to find unseen populations of exomoons, yet they have been unsuccessful. A plausible explanation is that most discovered planets are located on close-in orbits, which would make their moons prone
Externí odkaz:
http://arxiv.org/abs/1912.08049
Autor:
Sucerquia, Mario, Alvarado-Montes, Jaime A., Zuluaga, Jorge I., Cuello, Nicolás, Giuppone, Cristian
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 489, Issue 2, October 2019, Pages 2313-2322, https://doi.org/10.1093/mnras/stz2110
Close-in giant planets represent the most significant evidence of planetary migration. If large exomoons form around migrating giant planets which are more stable (e.g. those in the Solar System), what happens to these moons after migration is still
Externí odkaz:
http://arxiv.org/abs/1906.11400