Axi-symmetric models of B[e] supergiants: I. The effective temperature and mass-loss dependence of the hydrogen and helium ionization structure

Astronomy and Astrophysics

Volumn 478, Issue 2, 2008, Pages 543-551

  Zsargo J ^a   Hillier, D J ^a   Georgiev, L N ^b  

^a UNIVERSITY OF PITTSBURGH   (United States)

^b UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

Atomic processes; Outflows; Radiative transfer; Stars: early type; Stars: winds

Indexed keywords

ANALYTICAL CALCULATION; ATOMIC PROCESS; AXISYMMETRIC; CONTINUUM RADIATION; EFFECTIVE TEMPERATURE; EMISSION LINES; EQUATORIAL REGIONS; LEVEL POPULATIONS; MASS LOSS RATE; MASS-LOSS; MODEL PARAMETERS; NON-LTE; OUTFLOWS; RESONANCE LINE; STARS: EARLY-TYPE; STARS: WINDS; STELLAR ATMOSPHERES; STELLAR ENVELOPE;

BEHAVIORAL RESEARCH; COMPUTER SIMULATION; HELIUM; HYDROGEN; NUMERICAL METHODS; STARS; TEMPERATURE;

IONIZATION;

EID: 57349099276     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078293     Document Type: Article

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