Author: Pichierri Gabriele Morbidelli Alessandro Lai Dong
Publisher: Edp Sciences
E-ISSN: 1432-0746|605|issue|A23-A23
ISSN: 0004-6361
Source: Astronomy & Astrophysics, Vol.605, Iss.issue, 2017-09, pp. : A23-A23
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Related content
Eccentricity evolution in mean motion resonance andnon-radial solar wind
Astronomy & Astrophysics, Vol. 501, Iss. 1, 2009-07 ,pp. :
On the Super-Earths locked in the 3:2 mean-motion resonance
EAS Publications Series, Vol. 42, Iss. issue, 2010-04 ,pp. :
HD 60532, a planetary system in a 3:1 mean motion resonance
Astronomy & Astrophysics, Vol. 496, Iss. 2, 2009-03 ,pp. :
One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c
By Armstrong David J. Santerne Alexandre Veras Dimitri Barros Susana C. C. Demangeon Olivier Lillo-Box Jorge McCormac James Osborn Hugh P. Tsantaki Maria Almenara José-Manuel Barrado David Boisse Isabelle Bonomo Aldo S. Brown David J. A. Bruno Giovanni Cerda Javiera Rey Courcol Bastien Deleuil Magali Díaz Rodrigo F. Doyle Amanda P. Hébrard Guillaume Kirk James Lam Kristine W. F. Pollacco Don L. Rajpurohit Arvind Spake Jessica Walker Simon R.
Astronomy & Astrophysics, Vol. 582, Iss. issue, 2015-10 ,pp. :