Two-dimensional Monte Carlo simulations of H i line formation in massive young stellar object disc winds

Monthly Notices of the Royal Astronomical Society

Volumn 363, Issue 2, 2005, Pages 615-627

  Sim, S A ^a   Drew, J E ^a   Long, K S ^b  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b AURA for the European Space Agency   (United States)

Author keywords

Methods: numerical; Radiative transfer; Stars: early; Stars: winds, outflows; Type

Indexed keywords

INTELLIGENT SYSTEMS; MONTE CARLO METHODS; NUMERICAL METHODS; STARS;

INFRARED SPECTRUM; LINE FORMATIONS; METHOD: NUMERICAL; MONTE CARLO'S SIMULATION; RADIATIVE TRANSFER CALCULATIONS; STAR: EARLY; STARS: WINDS OUTFLOWS; TWO-DIMENSIONAL; TYPE; YOUNG STELLAR OBJECTS;

RADIATIVE TRANSFER;

EID: 27144540471     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09472.x     Document Type: Article

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