Mass determination of K2-19b and K2-19c from radial velocities and transit timing variations

We present radial velocity follow-up observations of K2-19, a compact planetary system hosting three planets, of which the two larger ones, K2-19b and K2-19c, are close to the 3:2 mean motion resonance.

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Bibliographic Details
Main Authors: Nespral, David (Author) , Gandolfi, Davide (Author)
Format: Article (Journal)
Language:English
Published: 19 May 2017
In: Astronomy and astrophysics
Year: 2017, Volume: 601
ISSN:1432-0746
DOI:10.1051/0004-6361/201628639
Online Access:Resolving-System, kostenfrei, Volltext: http://dx.doi.org/10.1051/0004-6361/201628639
Verlag, kostenfrei, Volltext: https://www.aanda.org/articles/aa/abs/2017/05/aa28639-16/aa28639-16.html
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Author Notes:D. Nespral, D. Gandolfi, H.J. Deeg, L. Borsato, M.C.V. Fridlund, O. Barragán, R. Alonso, S. Grziwa, J. Korth, S. Albrecht, J. Cabrera, Sz. Csizmadia, G. Nowak, T. Kuutma, J. Saario, P. Eigmüller, A. Erikson, E.W. Guenther, A.P. Hatzes, P. Montañés Rodríguez, E. Palle, M. Pätzold, J. Prieto-Arranz, H. Rauer and D. Sebastian
Description
Summary:We present radial velocity follow-up observations of K2-19, a compact planetary system hosting three planets, of which the two larger ones, K2-19b and K2-19c, are close to the 3:2 mean motion resonance.
Item Description:Gesehen am 22.08.2018
Physical Description:Online Resource
ISSN:1432-0746
DOI:10.1051/0004-6361/201628639