The broad Ha, [Oui] line wings in stellar supercluster A of NGC 2363 and the turbulent mixing layer hypothesis

Astronomy and Astrophysics

Volumn 500, Issue 2, 2009, Pages 817-826

  Binette, L ^a,b   Drissen, L ^a   Ubeda L ^a   Raga, A C ^b   Robert, C ^a   Krongold, Y ^b  

^a UNIVERSITÉ LAVAL   (Canada)

^b UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

Galaxies, clusters, general; Stars, formation; Ism, hii regions ; Line, profiles ; Stars, winds, outflows; Turbulence

Indexed keywords

- GALAXIES, CLUSTERS, GENERAL; - STARS, FORMATION; ALTERNATIVE PROCESS; BROAD LINE; CONSTANT ACCELERATION; EMISSION LINES; FIRST-ORDER; GAUSSIAN PROFILES; H II REGIONS; HIGH VELOCITY; ISM, HII REGIONS -; LINE EMISSIVITY; LINE SOURCES; LINE, PROFILES -; MIXING LENGTH APPROACH; RADIAL ACCELERATION; THREE DIMENSIONS; TURBULENT LAYER; TURBULENT MIXING LAYERS; WIND VELOCITIES;

ELECTROMAGNETIC WAVE EMISSION; GALAXIES; PHOTOIONIZATION; STARS; TIN; TURBULENCE;

LEAKAGE (FLUID);

EID: 67649548032     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811132     Document Type: Article

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