The Pan-Pacific Planet Search. IV. Two super-Jupiters in a 3:5
resonance orbiting the giant star HD 33844
Author
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Wittenmyer, Robert
Author
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Johnson, John
Author
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Butler, R.
Author
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Horner, Jonathan
Author
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Wang, Liang
Author
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Robertson, Paul
Author
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Jones, M.
Author
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Jenkins, James Stewart
Author
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Brahm, R.
Author
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Tinney, C.
Author
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Mengel, M.
Author
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Clark, J.
Admission date
dc.date.accessioned
2016-06-17T21:02:04Z
Available date
dc.date.available
2016-06-17T21:02:04Z
Publication date
dc.date.issued
2016
Cita de ítem
dc.identifier.citation
Astrophysical Journal Volumen: 818 Número: 1 Número de artículo: 35 (2016)
en_US
Identifier
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DOI: 10.3847/0004-637X/818/1/35
Identifier
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https://repositorio.uchile.cl/handle/2250/139017
General note
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Artículo de publicación ISi
en_US
Abstract
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We 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.