Results 1 - 10 of 2,294

Multiplicity Study of Exoplanet Host Stars

by M. Mugrauer, C. Ginski, T. Eisenbeiss
"... Abstract. We present recent results of our ongoing multiplicity study of exoplanet host stars. ..."
Abstract - Add to MetaCart
Abstract. We present recent results of our ongoing multiplicity study of exoplanet host stars.

On the Ages of Exoplanet Host Stars ⋆

by unknown authors , 2005
"... A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are: ..."
Abstract - Add to MetaCart
A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are:

gyrochronology for exoplanet host stars?

by D. J. A. Brown
"... ar ..."
Abstract - Add to MetaCart
Abstract not found

Abundances Stratification of Exoplanet Host Stars

by C. Saffe, H. Levato, Z. López-garcía, E. Jofré, R. Petrucci, E. González , 1492
"... Aims. To determineΣ(variation of Fe abundance with the optical depth),τFeI,τFeII (Rosseland median optical depth of Fe lines) and ∆[Fe/H](=[FeI/H]-[FeII/H]), in 79 Exoplanet Host stars (66 main sequence and 13 giants), with respect to 322 solar neighborhood field stars (9 main sequence and 313 giant ..."
Abstract - Add to MetaCart
Aims. To determineΣ(variation of Fe abundance with the optical depth),τFeI,τFeII (Rosseland median optical depth of Fe lines) and ∆[Fe/H](=[FeI/H]-[FeII/H]), in 79 Exoplanet Host stars (66 main sequence and 13 giants), with respect to 322 solar neighborhood field stars (9 main sequence and 313

Revising the ages of planet-hosting stars

by A. Bonfanti, S. Ortolani, G. Piotto, V. Nascimbeni , 2014
"... Aims. This article aims to measure the age of planet-hosting stars (SWP) through stellar tracks and isochrones computed with the PAdova & TR ieste Stellar Evolutionary Code (PARSEC). Methods. We developed algorithms based on two different techniques for determining the ages of field stars: isoch ..."
Abstract - Add to MetaCart
Aims. This article aims to measure the age of planet-hosting stars (SWP) through stellar tracks and isochrones computed with the PAdova & TR ieste Stellar Evolutionary Code (PARSEC). Methods. We developed algorithms based on two different techniques for determining the ages of field stars

The exoplanet-host star iota Horologii: an

by S. Vauclair, M. Laym, F. Bouchy, G. Vauclair, A. Hui, Bon Hoa, S. Charpinet, M. Bazot , 803
"... evaporated member of the primordial Hyades ..."
Abstract - Add to MetaCart
evaporated member of the primordial Hyades

FUNDAMENTAL PARAMETERS OF EXOPLANETS AND THEIR HOST STARS BY

by Jeffrey Langer Coughlin , 2012
"... ar ..."
Abstract - Add to MetaCart
Abstract not found

The Densities of Planets and Masses of Host Stars

by Eike W. Guenther
"... ar ..."
Abstract - Add to MetaCart
Abstract not found

Multiplicity in transiting planet host stars

by J. Lillo-box, D. Barrado, H. Bouy , 2012
"... ar ..."
Abstract - Add to MetaCart
Abstract not found

Binarity of Transit Host Stars ⋆ Implications on Planetary Parameters

by Sebastian Daemgen, Felix Hormuth, Wolfgang Br, Carolina Bergfors, Markus Janson, Thomas Henning , 2009
"... Context. Straight-forward derivation of planetary parameters can only be achieved in transiting planetary systems. However, planetary attributes such as radius and mass strongly depend on stellar host parameters. Discovering a transit host star to be multiple leads to a necessary revision of the der ..."
Abstract - Add to MetaCart
Context. Straight-forward derivation of planetary parameters can only be achieved in transiting planetary systems. However, planetary attributes such as radius and mass strongly depend on stellar host parameters. Discovering a transit host star to be multiple leads to a necessary revision
Results 1 - 10 of 2,294