Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/180733
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dc.contributor.advisorPerger, Manuel-
dc.contributor.advisorJordi i Nebot, Carme-
dc.contributor.authorBlanco Pozo, Jordi-
dc.date.accessioned2021-10-20T15:06:50Z-
dc.date.available2021-10-20T15:06:50Z-
dc.date.issued2021-07-
dc.identifier.urihttp://hdl.handle.net/2445/180733-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutors: Manuel Perger, Carme Jordi i Nebotca
dc.description.abstractThe LOFAR mission announced the detection of a radio emission coming from the M dwarf GJ 1151 which is consistent with the possible interaction of the star with an Earth-like exoplanet with an orbit of 1 to 5 d. Combining new data from different radial velocity surveys we calculate a new upper limit on the minimum mass of this possible companion at 0.9 M⊕ to 1.6 M⊕ for a 1.02 d to 5 d orbit. We also find evidence of a Neptune-like companion with a minimum mass of 10.6 ± 1.5 M⊕ on a 396 ± 6 d circular orbit and a likely more massive Neptunian exoplanet with a minimum mass of 24 ± 1.5 M⊕ on a 2093+130 d keplerian orbit.ca
dc.format.extent5 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Blanco, 2021-
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.subject.classificationGJ 1151cat
dc.subject.classificationPlanetes extrasolarscat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherGJ 1151eng
dc.subject.otherExtrasolar planetseng
dc.subject.otherBachelor's thesiseng
dc.titleNew insights on planetary companions of GJ 1151eng
dc.typeinfo:eu-repo/semantics/bachelorThesisca
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
Appears in Collections:Treballs Finals de Grau (TFG) - Física

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