Three planets around HD 27894: a close-in pair with a 2:1 period ratio and an eccentric Jovian planet at 5.4 AU
Aims. Our new program with HARPS aims to detect mean motion resonant planetary systems around stars which were previously reported to have a single bona fide planet, often based only on sparse radial velocity data. Methods. Archival and new HARPS radial velocities for the K2V star HD 27894 were comb...
Saved in:
| Main Authors: | , , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
June 5, 2017
|
| In: |
Arxiv
|
| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1706.00509 |
| Author Notes: | T. Trifonov, M. Kürster, M. Zechmeister, O.V. Zakhozhay, S. Reffert, M.H. Lee, F. Rodler, S.S. Vogt, and S.S. Brems |
Search Result 1