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Volumn 99, Issue 2, 1990, Pages 595-607

The evolution of the lithium abundances of solar-type stars. I. The Hyades and Coma Berenices clusters

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[No Author keywords available]

Indexed keywords


EID: 0001088108     PISSN: 00046256     EISSN: None     Source Type: Journal    
DOI: 10.1086/115353     Document Type: Article
Times cited : (120)

References (87)
  • 3
    • 85045492018 scopus 로고
    • The Impact of Very High S/N Spectroscopy on Stellar Physics, edited by G. Cayrel be Strobel and M. Spite (Kluwer, Dordrecht)
    • Baglin, A., and Morel, P.-J. (1988). In The Impact of Very High S/N Spectroscopy on Stellar Physics, IAU Symposium No. 132, edited by G. Cayrel be Strobel and M. Spite (Kluwer, Dordrecht), p. 279.
    • (1988) IAU Symposium No. 132 , pp. 279
    • Baglin, A.1    Morel, P.-J.2
  • 10
    • 85045493139 scopus 로고
    • The Impact of Very High S/N Spectroscopy on Stellar Physics, edited by G. Cayrel de Strobel and M. Spite (Kluwer, Dordrecht)
    • Boesgaard, A. M. (1988). In The Impact of Very High S/N Spectroscopy on Stellar Physics, IAU Symposium No. 132, edited by G. Cayrel de Strobel and M. Spite (Kluwer, Dordrecht), p. 386.
    • (1988) IAU Symposium No. 132 , pp. 386
    • Boesgaard, A.M.1
  • 46
    • 0011575710 scopus 로고
    • Observational Tests of the Stellar Evolution Theory, edited by A. Maeder and A. Renzini (Reidel, Dordrecht)
    • Mayor, M., and Mermilliod, J.-C. (1984). In Observational Tests of the Stellar Evolution Theory, IAU Symposium No. 105, edited by A. Maeder and A. Renzini (Reidel, Dordrecht), p. 411.
    • (1984) IAU Symposium No. 105 , pp. 411
    • Mayor, M.1    Mermilliod, J.-C.2
  • 67
    • 85045488049 scopus 로고
    • The Impact of Very High S/N Spectroscopy on Steller Physics, edited by G. Cayrel de Strobel and M. Spite (Kluwer, Dordrecht)
    • Soderblom, D. R. (1988). In The Impact of Very High S/N Spectroscopy on Steller Physics, IAU Symposium No. 132, edited by G. Cayrel de Strobel and M. Spite (Kluwer, Dordrecht), p. 381.
    • (1988) IAU Symposium No. 132 , pp. 381
    • Soderblom, D.R.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.