Transiting Sub-stellar companions of Intermediate-mass stars

We use the CoRoT-survey to search for transiting close-in planets of intermediate-mass stars (M* = 1.3 − 2.1 M⊙). We present recent results of our survey. RV-surveys and direct imaging campaigns showed, that intermediate-mass main-sequence stars have more massive planets then solar-like stars. Even...

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Main Authors: Sebastian Daniel, Guenther Eike W., Heber Ulrich, Geier Stephan, Grziwa Sascha
Format: Article
Language:English
Published: EDP Sciences 2015-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/201510106056
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author Sebastian Daniel
Guenther Eike W.
Heber Ulrich
Geier Stephan
Grziwa Sascha
author_facet Sebastian Daniel
Guenther Eike W.
Heber Ulrich
Geier Stephan
Grziwa Sascha
author_sort Sebastian Daniel
collection DOAJ
description We use the CoRoT-survey to search for transiting close-in planets of intermediate-mass stars (M* = 1.3 − 2.1 M⊙). We present recent results of our survey. RV-surveys and direct imaging campaigns showed, that intermediate-mass main-sequence stars have more massive planets then solar-like stars. Even brown dwarfs have been found. In our study we concentrated on short-period planets for which a mass-determination is possible. The detection of close-in planets of intermediate-mass stars put strong constraints on the timescales of the formation and migration. We already have identified transiting Jupiter-like planet candidates with short orbital periods and observed these candidates with high-resolution echelle-spectrographs at various Telescopes.
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spelling doaj.art-8736bd1e967f44659686a78aae5c1e172022-12-21T22:15:25ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-011010605610.1051/epjconf/201510106056epjconf_sphr2014_06056Transiting Sub-stellar companions of Intermediate-mass starsSebastian DanielGuenther Eike W.Heber UlrichGeier StephanGrziwa SaschaWe use the CoRoT-survey to search for transiting close-in planets of intermediate-mass stars (M* = 1.3 − 2.1 M⊙). We present recent results of our survey. RV-surveys and direct imaging campaigns showed, that intermediate-mass main-sequence stars have more massive planets then solar-like stars. Even brown dwarfs have been found. In our study we concentrated on short-period planets for which a mass-determination is possible. The detection of close-in planets of intermediate-mass stars put strong constraints on the timescales of the formation and migration. We already have identified transiting Jupiter-like planet candidates with short orbital periods and observed these candidates with high-resolution echelle-spectrographs at various Telescopes.http://dx.doi.org/10.1051/epjconf/201510106056
spellingShingle Sebastian Daniel
Guenther Eike W.
Heber Ulrich
Geier Stephan
Grziwa Sascha
Transiting Sub-stellar companions of Intermediate-mass stars
EPJ Web of Conferences
title Transiting Sub-stellar companions of Intermediate-mass stars
title_full Transiting Sub-stellar companions of Intermediate-mass stars
title_fullStr Transiting Sub-stellar companions of Intermediate-mass stars
title_full_unstemmed Transiting Sub-stellar companions of Intermediate-mass stars
title_short Transiting Sub-stellar companions of Intermediate-mass stars
title_sort transiting sub stellar companions of intermediate mass stars
url http://dx.doi.org/10.1051/epjconf/201510106056
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AT geierstephan transitingsubstellarcompanionsofintermediatemassstars
AT grziwasascha transitingsubstellarcompanionsofintermediatemassstars