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Abstract

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We present a new database of stellar evolution models for a large range of masses and chemical compositions, based on an up-to-date theoretical framework. We briefly discuss the physical inputs and the assumptions adopted in computing the stellar models. We explain how to access to the on-line archive and briefly discuss the interactive WEB tools that can be used to compute user-specified evolutionary tracks/isochrones/luminosity functions. The future developments of this database are also outlined.

Details

1009240
Subject
Stellar evolution;
Luminosity;
Organic chemistry;
Chemical composition;
Astronomical models;
Stellar models;
Databases
URL
http://arxiv.org/abs/astro-ph/0509543
Title
BASTI: An interactive database of updated stellar evolution models
Author
Cassisi, S; Pietrinferni, A; Salaris, M; Castelli, F; Cordier, D; Castellani, M
Publication title
arXiv.org; Ithaca
Publication year
2005
Publication date
Sep 19, 2005
Section
Astrophysics
Publisher
Cornell University Library, arXiv.org
Source
arXiv.org
Place of publication
Ithaca
Country of publication
United States
University/institution
Cornell University Library arXiv.org
Publication subject
Biology, Statistics, Physics, Mathematics, Engineering--Electrical Engineering, Computers--Computer Engineering, Business And Economics--Banking And Finance
e-ISSN
2331-8422
Source type
Working Paper
Language of publication
English
Document type
Working Paper
Publication history
 
 
Online publication date
2010-12-09
Milestone dates
2005-09-19 (Submission v1)
Publication history
 
 
   First posting date
09 Dec 2010
ProQuest document ID
2087291105
Document URL
https://www.proquest.com/working-papers/basti-interactive-database-updated-stellar/docview/2087291105/se-2?accountid=130970
Full text outside of ProQuest
http://arxiv.org/abs/astro-ph/0509543
Copyright
Notwithstanding the ProQuest Terms and conditions, you may use this content in accordance with the associated terms available at http://arxiv.org/abs/astro-ph/0509543.
Last updated
2020-03-11
Database
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