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Authordc.contributor.authorJenkins, James Stewart 
Authordc.contributor.authorJones, H. R.A. 
Authordc.contributor.authorTuomi, M. 
Authordc.contributor.authorDíaz, M. 
Authordc.contributor.authorCordero, J. P. 
Authordc.contributor.authorAguayo, A. 
Authordc.contributor.authorPantoja, B. 
Authordc.contributor.authorArriagada, P. 
Authordc.contributor.authorMahu, R. 
Authordc.contributor.authorBrahm, R. 
Authordc.contributor.authorRojo, P. 
Authordc.contributor.authorSoto, M. G. 
Authordc.contributor.authorIvanyuk, O. 
Authordc.contributor.authorBecerra Yoma, Néstor 
Authordc.contributor.authorDay-Jones, A. C. 
Authordc.contributor.authorRuiz, M. T. 
Authordc.contributor.authorPavlenko, Y. V. 
Authordc.contributor.authorBarnes, J. R. 
Authordc.contributor.authorMurgas, F. 
Authordc.contributor.authorPinfield, D. J. 
Admission datedc.date.accessioned2019-05-29T13:30:04Z
Available datedc.date.available2019-05-29T13:30:04Z
Publication datedc.date.issued2017
Cita de ítemdc.identifier.citationMonthly Notices of the Royal Astronomical Society, Volumen 466, Issue 1, 2017, Pages 443-473
Identifierdc.identifier.issn13652966
Identifierdc.identifier.issn00358711
Identifierdc.identifier.other10.1093/mnras/stw2811
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/168899
Abstractdc.description.abstractWe report the discovery of eight new giant planets, and updated orbits for four known planets,orbiting dwarf and subgiant stars using the CORALIE, HARPS, and MIKE instruments aspart of the Calan–Hertfordshire Extrasolar Planet Search. The planets have masses in therange 1.1–5.4MJ’s, orbital periods from 40 to 2900 d, and eccentricities from 0.0 to 0.6. Theyinclude a double-planet system orbiting the most massive star in our sample (HD147873),two eccentric giant planets (HD128356band HD154672b), and a rare 14 Herculis analogue(HD224538b). We highlight some population correlations from the sample of radial velocitydetected planets orbiting nearby stars, including the mass function exponential distribution,confirmation of the growing body of evidence that low-mass planets tend to be found orbitingmore metal-poor stars than giant planets, and a possible period–metallicity correlation forplanets with masses>0.1MJ, based on a metallicity difference of 0.16 dex between thepopulation of planets with orbital periods less than 100 d and those with orbital periods greaterthan 100 d.
Lenguagedc.language.isoen
Publisherdc.publisherOxford University
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
Sourcedc.sourceMonthly Notices of the Royal Astronomical Society
Keywordsdc.subjectPlanetary systems
Keywordsdc.subjectPlanets and satellites: formation
Keywordsdc.subjectStars: activity
Keywordsdc.subjectStars: low-mass
Keywordsdc.subjectStars: solar-type
Títulodc.titleNew planetary systems from the Calan-Hertfordshire Extrasolar planet search
Document typedc.typeArtículo de revista
Catalogueruchile.catalogadorlaj
Indexationuchile.indexArtículo de publicación SCOPUS
uchile.cosechauchile.cosechaSI


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Attribution-NonCommercial-NoDerivs 3.0 Chile
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