Non-local thermodynamic equilibrium effects in modelling of Supernovae near maximum light
Author(s) -
E. Baron,
P. H. Hauschildt,
P. Nugent,
David Branch
Publication year - 1996
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1093/mnras/283.1.297
Subject(s) - physics , supernova , opacity , astrophysics , spectral line , blanketing , thermodynamic equilibrium , line (geometry) , metallicity , ionization , radiative transfer , stars , thermodynamics , astronomy , quantum mechanics , ion , geometry , mathematics
Supernovae (SNe), with their diversity of compositions, velocities, envelope masses, and interactions, are good testing grounds for probing the importance of non-local thermodynamic equilibrium (NLTE) in expanding atmospheres. In addition to treating H, He, Li I, O I, Ne I, Na I, and Mg II in NLTE, we use a very large model atom of Fe II to test the importance of NLTE processes in both Type Ia and...
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