Low temperature Rosseland opacities with varied abundances of carbon and nitrogen

Astronomy and Astrophysics

Volumn 494, Issue 1, 2009, Pages 403-416

  Lederer, M T ^a   Aringer, B ^a,b  

^a UNIVERSITY OF VIENNA   (Austria)

^b UNIVERSITY OF PADOVA   (Italy)

Author keywords

Molecular data; Radiative transfer; Stars: evolution

Indexed keywords

ASTROPHYSICS; ATOMIC PHYSICS; CARBON MONOXIDE; CHEMICAL ELEMENTS; GEOPHYSICS; MOLECULAR OXYGEN; MOLECULES; NITROGEN; NONMETALS; OXYGEN; PHASE EQUILIBRIA; RADIATION; RADIATIVE TRANSFER; SOLAR ENERGY; STARS;

A CARBONS; ASTROPHYSICAL APPLICATIONS; ATOMIC LINES; CARBON AND NITROGENS; CARBON-RICH; CHEMICAL COMPOSITIONS; CHEMICAL EQUILIBRIUM CALCULATIONS; CO MOLECULES; DATA SETS; DIFFUSION APPROXIMATIONS; HEAVY ELEMENTS; INITIAL SITUATIONS; INPUT DATUM; LOW TEMPERATURES; METALLICITIES; METALLICITY; MOLECULAR DATA; MOLECULAR LINES; NEUTRAL ATOMS; ORDERS OF MAGNITUDES; OTHER APPLICATIONS; PARAMETER RANGES; RADIATIVE ENERGIES; ROSSELAND MEAN OPACITIES; STARS: EVOLUTION; STELLAR EVOLUTIONS; TEMPERATURE RANGES;

OPACITY;

EID: 59449096058     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810576     Document Type: Article

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