Computer Science
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1725f&link_type=abstract
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1725
Computer Science
Scientific paper
Up to now more than 500 extra-solar planets have been discovered. Many of these extrasolar systems consist of one star and only one massive, near-by giant planet. However, recently more and more different types of systems become known, including also extrasolar planets in binaries. In our study we will concentrate on planetary systems in binaries, since a large percentage of all G-M stars are expected to be part of binary or multiple stellar systems. Therefore, these kinds of systems are worth to be investigated in detail. In particular we will concentrate on planets in PType motion. During the last years four such systems (NN Ser, HW Vir, HU Aqr and DP Leo) have been discovered. In our study we perform dynamical studies, where we compare simulated eclipse timing variations (ETV) to current observational data and found out, that the proposed system configurations are highly unlikely.
Eggl Siegfried
Funk Barbara
Gyergyovits Markus
Pilat-Lohinger Elke
Schwarz Ralf
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