dc.creatorFernández Lajús, Eduardo
dc.creatorMiguel, Yamila
dc.creatorFortier, Andrea
dc.creatorDi Sisto, Romina Paula
dc.date2010
dc.date2019-10-03T16:10:50Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/82624
dc.identifierissn:1743-9213
dc.descriptionPhotometric observations of transits can be used to derive physical and orbital parameters of the system, like the planetary and stellar radius, orbital inclination and mean density of the star. Furthermore, monitoring possible periodic variations in transit timing of planets is important, since small changes can be caused by the presence of other planets or moons in the system. On the other hand, long term changes in the transit length can be due to the orbital precession of the planets. For these reasons we started an observational program dedicated to observe transits of known exoplanets with the aim of contributing to a better understanding of these planetary systems. In this work we present our first results obtained using the observational facilities in Argentina including the 2.15 telescope at CASLEO.
dc.descriptionInstituto de Astrofísica de La Plata
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format416-417
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectPlanetary systems
dc.subjectStars: variables: other
dc.subjectTechniques: photometric
dc.titleMonitoring and analyzing exoplanetary transits from Argentina
dc.typeArticulo
dc.typeArticulo


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