On the stability of radiation-pressure-dominated cavities

Astronomy and Astrophysics

Volumn 537, Issue , 2012, Pages

  Kuiper, R ^a,b   Klahr, H ^b   Beuther, H ^b   Henning, Th ^b  

^a UNIVERSITY OF BONN   (Germany)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

hydrodynamics; methods: numerical; radiative transfer; stars: formation; stars: massive; stars: winds, outflows

Indexed keywords

ANALYTICAL MODEL; FUNDAMENTAL PROPERTIES; GRAVITATIONAL ATTRACTION; INITIAL DENSITY; MASSIVE STARS; METHODS: NUMERICALS; ORDERS OF MAGNITUDE; RADIATION HYDRODYNAMICS SIMULATION; RADIATION PRESSURE; RADIATION TRANSPORT; RADIATIVE FORCES; RAYLEIGH-TAYLOR INSTABILITIES; STARS: FORMATION; STARS: MASSIVE; STARS: WINDS, OUTFLOWS; STELLAR IRRADIATION; STELLAR RADIATION;

COMPUTER SIMULATION; HYDRODYNAMICS; IRRADIATION; MATHEMATICAL MODELS; PRESSURE; RADIATIVE TRANSFER; RAYLEIGH SCATTERING; SHELLS (STRUCTURES); STABILITY; STARS;

RADIATION;

EID: 84855928367     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117808     Document Type: Article

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