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T Tauri Disk Lifetime in the Lupus Association

Published online by Cambridge University Press:  27 January 2016

P. A. B. Galli ,
C. Bertout ,
R. Teixeira  and
C. Ducourant
P. A. B. Galli
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão, 1226 - Cidade Universitária, 05508-900, São Paulo - SP, Brazil. email: [email protected]
C. Bertout
Affiliation:
Institut d'Astrophysique, 98bis, Bd. Arago, 75014 Paris, France.
R. Teixeira
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão, 1226 - Cidade Universitária, 05508-900, São Paulo - SP, Brazil. email: [email protected]
C. Ducourant
Affiliation:
Univ. Bordeaux, LAB, UMR 5804, F-33270, Floirac, France. Observatoire Aquitain des Sciences de l'Univers, CNRS-UMR 5804, 33270 Floirac, France.
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Abstract

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In a recent study, we derived individual distances for a sample of pre-main sequence stars that define the comoving association of young stars in the Lupus star-forming region. Here, we use these new distances to investigate the mass and age distributions of Lupus T Tauri stars and derive the average disk lifetime in the Lupus association based on an empirical disk model.

Keywords

stars: variables: T TauriHerbig Ae/Be - stars: formation - stars: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S314: Young Stars & Planets Near the Sun , November 2015 , pp. 191 - 192
Copyright
Copyright © International Astronomical Union 2016 

References

Bertout, C. 1989, ARA&A, 27, 351Google Scholar
Bertout, C., Siess, L., & Cabrit, S. 2007, A&A, 473, L21Google Scholar
Galli, P. A. B., Bertout, C., Teixeira, R., & Ducourant, C. 2013, A&A, 558, A77Google Scholar
Siess, L., Dufour, E., & Forestini, M. 2000, A&A, 358, 593Google Scholar