Mostrar el registro sencillo del ítem

dc.contributor.author
Lillo Box, J.  
dc.contributor.author
Demangeon, O.  
dc.contributor.author
Santerne, A.  
dc.contributor.author
Barros, S. C. C.  
dc.contributor.author
Barrado, D.  
dc.contributor.author
Hébrard, G.  
dc.contributor.author
Osborn, H. P.  
dc.contributor.author
Armstrong, D. J.  
dc.contributor.author
Almenara, J. M.  
dc.contributor.author
Boisse, I.  
dc.contributor.author
Bouchy, F.  
dc.contributor.author
Brown, D. J. A.  
dc.contributor.author
Courcol, B.  
dc.contributor.author
Deleuil, M.  
dc.contributor.author
Delgado Mena, E.  
dc.contributor.author
Diaz, Rodrigo Fernando  
dc.contributor.author
Kirk, J.  
dc.contributor.author
Lam, K. W. F.  
dc.contributor.author
McCormac, J.  
dc.contributor.author
Pollacco, D.  
dc.contributor.author
Rajpurohit, A.  
dc.contributor.author
Rey, J.  
dc.contributor.author
Santos, N. C.  
dc.contributor.author
Sousa, S. G.  
dc.contributor.author
Tsantaki, M.  
dc.contributor.author
Wilson, P. A.  
dc.date.available
2017-06-19T18:28:07Z  
dc.date.issued
2016-10  
dc.identifier.citation
Lillo Box, J.; Demangeon, O.; Santerne, A.; Barros, S. C. C.; Barrado, D.; et al.; K2-30 b and K2-34 b: Two inflated hot Jupiters around solar-type stars; Edp Sciences; Astronomy And Astrophysics; 594; A50; 10-2016; 1-7  
dc.identifier.issn
0004-6361  
dc.identifier.uri
http://hdl.handle.net/11336/18444  
dc.description.abstract
We report the discovery of the two hot Jupiters K2-30 b and K2-34 b. The two planets were detected during campaigns 4 and 5 of the extension of the Kepler mission, K2; they transit their main-sequence stars with periods of ~4.099 and ~2.996 days. Subsequent ground-based radial velocity follow-up with SOPHIE, HARPS-N, and CAFE established the planetary nature of the transiting objects. We analyzed the transit signal, radial velocity, and spectral energy distributions of the two systems to characterize their properties. Both planets (K2-30 b and K2-34 b) are bloated hot Jupiters (1.20 RJup and 1.22 RJup) around relatively bright (V = 13.5 and V = 11.5) slow rotating main-sequence (G8 and F9) stars. Thus, these systems are good candidates for detecting the Rossiter-MacLaughlin effect in order to measure their obliquity and for atmospheric studies.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
Edp Sciences  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Planets And Satellites: Detection  
dc.subject
Planets And Satellites: Gaseous Planets  
dc.subject
Techniques: Radial Velocities  
dc.subject
Techniques: Photometric  
dc.subject
Techniques: High Angular Resolution  
dc.subject.classification
Astronomía  
dc.subject.classification
Ciencias Físicas  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
K2-30 b and K2-34 b: Two inflated hot Jupiters around solar-type stars  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2017-06-13T14:14:48Z  
dc.journal.volume
594  
dc.journal.number
A50  
dc.journal.pagination
1-7  
dc.journal.pais
Francia  
dc.journal.ciudad
Paris  
dc.description.fil
Fil: Lillo Box, J.. Centro de Astrobiología; España  
dc.description.fil
Fil: Demangeon, O.. Aix Marseille Université,; Francia  
dc.description.fil
Fil: Santerne, A.. Universidade do Porto,; Portugal  
dc.description.fil
Fil: Barros, S. C. C.. Universidade do Porto,; Portugal  
dc.description.fil
Fil: Barrado, D.. Centro de Astrobiología; España  
dc.description.fil
Fil: Hébrard, G.. Université Pierre & Marie Curie; Francia  
dc.description.fil
Fil: Osborn, H. P.. University Of Warwick; Reino Unido  
dc.description.fil
Fil: Armstrong, D. J.. University Of Warwick; Reino Unido  
dc.description.fil
Fil: Almenara, J. M.. Université Grenoble Alpes; Francia  
dc.description.fil
Fil: Boisse, I.. Aix Marseille Université; Francia  
dc.description.fil
Fil: Bouchy, F.. Aix Marseille Université; Francia  
dc.description.fil
Fil: Brown, D. J. A.. University Of Warwick; Reino Unido  
dc.description.fil
Fil: Courcol, B.. University Of Warwick; Reino Unido  
dc.description.fil
Fil: Deleuil, M.. Aix Marseille Université; Francia  
dc.description.fil
Fil: Delgado Mena, E.. Universidade do Porto; Portugal  
dc.description.fil
Fil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina  
dc.description.fil
Fil: Kirk, J.. University Of Warwick; Reino Unido  
dc.description.fil
Fil: Lam, K. W. F.. University Of Warwick; Reino Unido  
dc.description.fil
Fil: McCormac, J.. University Of Warwick; Reino Unido  
dc.description.fil
Fil: Pollacco, D.. University Of Warwick; Reino Unido  
dc.description.fil
Fil: Rajpurohit, A.. Aix Marseille Université,; Francia  
dc.description.fil
Fil: Rey, J.. Observatoire Astronomique de l’Université de Genève; Suiza  
dc.description.fil
Fil: Santos, N. C.. Universidade do Porto; Portugal  
dc.description.fil
Fil: Sousa, S. G.. Universidade do Porto; Portugal  
dc.description.fil
Fil: Tsantaki, M.. Universidade do Porto; Portugal  
dc.description.fil
Fil: Wilson, P. A.. Université Pierre & Marie Curie; Francia  
dc.journal.title
Astronomy And Astrophysics  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1051/0004-6361/201628204  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1601.07635  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2016/10/aa28204-16/aa28204-16.html  

Archivos asociados
Thumbnail
 
Tamaño: 550.9Kb
Formato: PDF
.