The discovery of a planetary candidate around the evolved low-mass Kepler giant star HD 175370
Artikel i vetenskaplig tidskrift, 2017
stars: individual: HD 175370 (KIC 007940959)
methods: data analysis
techniques: radial velocities
methods: observational
techniques: spectroscopic
planetary systems
Författare
M. Hrudkova
Isaac Newton Group
A. Hatzes
Thüringer Landessternwarte Tautenburg
R. Karjalainen
Isaac Newton Group
H. Lehmann
Thüringer Landessternwarte Tautenburg
S. Hekker
Max-Planck-Gesellschaft
Aarhus Universitet
M. Hartmann
Thüringer Landessternwarte Tautenburg
A. Tkachenko
KU Leuven
S. Prins
KU Leuven
H. van Winckel
KU Leuven
R. De Nutte
Royal Observatory of Belgium
L. Dumortier
Royal Observatory of Belgium
Y. Fremat
Royal Observatory of Belgium
H. Hensberge
Royal Observatory of Belgium
A. Jorissen
Université libre de Bruxelles (ULB)
P. Lampens
Royal Observatory of Belgium
M. Laverick
KU Leuven
Robin Lombaert
Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium
P. I. Papics
KU Leuven
G. Raskin
KU Leuven
A. Sodor
Royal Observatory of Belgium
Magyar Tudomanyos Akademia
A. Thoul
Kavli Institute for Theoretical Physics
Universite de Liège
S. Van Eck
Université libre de Bruxelles (ULB)
C. Waelkens
KU Leuven
Monthly Notices of the Royal Astronomical Society
0035-8711 (ISSN) 1365-2966 (eISSN)
Vol. 464 1 1018-1028Ämneskategorier
Astronomi, astrofysik och kosmologi
DOI
10.1093/mnras/stw2379