Sign on

SAO/NASA ADS Astronomy Abstract Service

· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· arXiv e-print (arXiv:0803.2505)
· References in the article
· Citations to the Article (13) (Citation History)
· Refereed Citations to the Article
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
Grids of stellar evolution models for asteroseismology ( cesam + posc)
Authors:
Marques, João P.; Monteiro, Mário J. P. F. G.; Fernandes, João M.
Affiliation:
AA(Centro de Astrofísica da Universidade do Porto;, Grupo de Astrofísica da Universidade de Coimbra), AB(Centro de Astrofísica da Universidade do Porto; Departamento de Matemática Aplicada da Faculdade de Ciências, Universidade do Porto), AC(Grupo de Astrofísica da Universidade de Coimbra; Departamento de Matemática da Faculdade de Ciências e Tecnologia, Universidade de Coimbra)
Publication:
Astrophysics and Space Science, Volume 316, Issue 1-4, pp. 173-178 (Ap&SS Homepage)
Publication Date:
08/2008
Origin:
SPRINGER
Keywords:
Stars: evolution, Stars: interiors, Stars: oscillations
DOI:
10.1007/s10509-008-9786-7
Bibliographic Code:
2008Ap&SS.316..173M

Abstract

In this paper we present a grid of stellar evolution models, computed with an up-to-date physical description of the internal structure, using the Code d'Évolution Stellaire Adaptatif et Modulaire ( cesam). The evolutionary sequences span from the pre-main sequence to the beginning of the Red Giant Branch and cover an interval of mass typical for low and intermediate mass stars. The chemical composition (both helium and metal abundance) is the solar one. The frequencies of oscillation, computed for specific stellar models of the grid using the Porto Oscillations Code ( posc), are also provided. This work was accomplished in order to support the preparation of the CoRoT mission within the Evolution and Seismic Tools Activity (CoRoT/ESTA). On the other hand, the grid can also be used, more generally, to interpret the observational properties of either individual stars or stellar populations. The grids (data and documentation) can be found at http://www.astro.up.pt/corot/models/cesam.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)
  New!

Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints