Show simple item record

Authordc.contributor.authorWittenmyer, Robert 
Authordc.contributor.authorJohnson, John 
Authordc.contributor.authorButler, R. 
Authordc.contributor.authorHorner, Jonathan 
Authordc.contributor.authorWang, Liang 
Authordc.contributor.authorRobertson, Paul 
Authordc.contributor.authorJones, M. 
Authordc.contributor.authorJenkins, James Stewart 
Authordc.contributor.authorBrahm, R. 
Authordc.contributor.authorTinney, C. 
Authordc.contributor.authorMengel, M. 
Authordc.contributor.authorClark, J. 
Admission datedc.date.accessioned2016-06-17T21:02:04Z
Available datedc.date.available2016-06-17T21:02:04Z
Publication datedc.date.issued2016
Cita de ítemdc.identifier.citationAstrophysical Journal Volumen: 818 Número: 1 Número de artículo: 35 (2016)en_US
Identifierdc.identifier.otherDOI: 10.3847/0004-637X/818/1/35
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/139017
General notedc.descriptionArtículo de publicación ISien_US
Abstractdc.description.abstractWe report the discovery of two giant planets orbiting the K giant HD 33844 based on radial velocity data from three independent campaigns. The planets move on nearly circular orbits with semimajor axes a(b) = 1.60 +/- 0.02 AU and a(c) = 2.24 +/- 0.05 AU, and have minimum masses (m sin i) of M-b = 1.96 +/- 0.12 M-Jup and M-c = 1.76 +/- 0.18 M-Jup. Detailed N- body dynamical simulations show that the two planets have remained on stable orbits for more than 10(6) years for low eccentricities and are most likely trapped in a mutual 3:5 mean motion resonance.en_US
Patrocinadordc.description.sponsorshipAustralian Research Council DP0774000 DP130102695en_US
Lenguagedc.language.isoenen_US
Publisherdc.publisherIOP PUBLISHINGen_US
Type of licensedc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Keywordsdc.subjectplanetary systemsen_US
Keywordsdc.subjectstars: individual (HD 33844)en_US
Keywordsdc.subjecttechniques: radial velocitiesen_US
Títulodc.titleThe Pan-Pacific Planet Search. IV. Two super-Jupiters in a 3:5 resonance orbiting the giant star HD 33844en_US
Document typedc.typeArtículo de revista


Files in this item

Icon

This item appears in the following Collection(s)

Show simple item record

Atribución-NoComercial-SinDerivadas 3.0 Chile
Except where otherwise noted, this item's license is described as Atribución-NoComercial-SinDerivadas 3.0 Chile