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Physical parameters for the EXPORT sample. Rotational velocities and effective temperatures

Published online by Cambridge University Press:  26 May 2016

E. Solano ,
B. Montesinos ,
A. Mora  and
EXPORT Team (A. Alberdi, A. Collier Cameron, J.K. Davies, H.J. Deeg, C. Eiroa, R. Ferlet, F. Garzon, C.A. Grady, A. Harris, K. Horne, B. Merfn, L.F. Miranda, R. Oudmaijer, J. Palacios, A. Penny, A. Quirrenbach, H. Rauer, J. Schneider, Y. Tsapras, P.R. Wesselius, D. de Winter
E. Solano
Affiliation:
INSA-LAEFF. Apartado de Correos 50727, E-28080 Madrid, Spain
B. Montesinos
Affiliation:
LAEFF. Apartado de Correos 50727, E-28080, Madrid, Spain Instituto de Astrofísica de Andalucía. CSIC Apartado de Correos 3004, E-18080, Granada, Spain
A. Mora
Affiliation:
Departamento de Física Teórica, Facultad de Ciencias, Universidad Autónoma de Madrid, E-28049 Cantoblanco, Madrid, Spain

Abstract

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The methods used to calculate projected rotational velocities and effective temperatures for the targets observed during the 1998-1999 La Palma International Time campaign are described here. This is part of a project whose main goal is to perform a detailed chemical analysis of these objects and to study their potential implications in the planetary formation phenomenon.

Type
Part I: Discovery and study of extrasolar planets - current
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 127 - 129
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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