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dc.date.accessioned 2019-10-03T16:07:12Z
dc.date.available 2019-10-03T16:07:12Z
dc.date.issued 2010
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/82623
dc.description.abstract With the end of answer questions as, how common are planetary systems like our own in the Universe? and What is the diversity of planetary systems that we could find in the universe?, we develop a semi-analytical model for computing planetary systems formation and consider different initial conditions for generating a large sample of planetary systems, which is analysed statistically. We explore the effects in the planetary system architecture of assuming different initial disc profiles and planetary migration rates. en
dc.format.extent 441-442 es
dc.language en es
dc.subject Planetary systems: formation es
dc.subject Planets and satellites: formation es
dc.title Planetary systems formation and the diversity of extrasolar systems en
dc.type Articulo es
sedici.identifier.other eid:2-s2.0-84883041489 es
sedici.identifier.other doi:10.1017/S1743921311020710 es
sedici.identifier.issn 17439213 es
sedici.creator.person Miguel, Yamila es
sedici.creator.person Guilera, Octavio Miguel es
sedici.creator.person Brunini, Adrián es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
mods.originInfo.place Instituto de Astrofísica de La Plata es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.event IAU Symposium 276 (Torino, Italy, 2010) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Proceedings of the International Astronomical Union es
sedici.relation.journalVolumeAndIssue vol. 6, no. S276 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)