Open AccessThe Mixing Length in Convective Stellar Envelopes is Proportional to Distance from the Convective Boundary
Author(s) -
Richard B. Stothers,
Chao-Wen Chin
Publication year - 1997
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/310552
Subject(s) - physics , astrophysics , mixing length model , convection , length scale , turbulence , convection zone , stellar mass , scale height , stellar atmosphere , stars , mechanics , star formation
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