Planets Around Active Stars View Full Text


Ontology type: schema:Chapter      Open Access: True


Chapter Info

DATE

2008

AUTHORS

J. Setiawan , P. Weise , Th. Henning , A. P. Hatzes , L. Pasquini , L. da Silva , L. Girardi , O. von der Lühe , M. P. Döllinger , A. Weiss , K. Biazzo

ABSTRACT

We present the results of radial velocity measurements of two samples of active stars. The first sample contains field G and K giants across the Red Giant Branch, whereas the second sample consists of nearby young stars (d < 150 pc) with ages between 10 and 300 Myrs. The radial velocity monitoring program has been carried out with FEROS at 1.52 m ESO telescope (1999 – 2002) and continued since 2003 at 2.2 m MPG/ESO telescope. We observed stellar radial velocity variations which originate either from the stellar activity or the presence of stellar/substellar companions. By means of a bisector technique we are able to distinguish the sources of the radial velocity variation. Among them we found few candidates of planetary companions, both of young stars and G-K giants sample. More... »

PAGES

201-204

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-3-540-75485-5_43

DOI

http://dx.doi.org/10.1007/978-3-540-75485-5_43

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1044769036


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