New pre-main-sequence tracks for M ≤ 2.5 M⊙ as tests of opacities and convection model

Astrophysical Journal, Supplement Series

Volumn 90, Issue 1, 1994, Pages 467-500

  D'Antona, Francesca ^a   Mazzitelli, Italo ^b  

^a INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

Author keywords

Atomic processes; Convection; Stars: abundances; Stars: interiors; Stars: pre main sequence

Indexed keywords

EID: 12044253692     PISSN: 00670049     EISSN: None     Source Type: Journal    
DOI: 10.1086/191867     Document Type: Article

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