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Astronomy and Astrophysics

Volumn 383, Issue 3, 2002, Pages 1113-1124

Emission profile variability in hot star winds: A pseudo-3D method based on radiation hydrodynamics simulations

(2) Dessart, L a Owocki, S P b

a UTRECHT UNIVERSITY (Netherlands)

b UNIVERSITY OF DELAWARE (United States)

Author keywords

Line: formation; Radiative transfer; Stars: atmospheres; Stars: early type; Stars: mass loss

Indexed keywords

COMPUTER SIMULATION; ELECTROMAGNETIC WAVE EMISSION; HYDRODYNAMICS; SIGNAL TO NOISE RATIO;

HOT STAR WINDS;

ASTROPHYSICS;

EID: 0036492471 PISSN: 00046361 EISSN: None Source Type: Journal
DOI: 10.1051/0004-6361:20011826 Document Type: Article

Times cited : (45)

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