Feedback by massive stars and the emergence of superbubbles: I. Energy efficiency and Vishniac instabilities

Astronomy and Astrophysics

Volumn 550, Issue , 2013, Pages

  Krause, M ^a,b   Fierlinger, K ^a,c   Diehl, R ^a,b   Burkert, A ^b,c,d   Voss, R ^e   Ziegler, U ^f  

^a EXCELLENCE CLUSTER UNIVERSE   (Germany)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c UNIVERSITY OF MUNICH   (Germany)

^d Max Planck Fellow ^*  (Germany)

^e RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

^f ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

Author keywords

Galaxies: ISM; Hydrodynamics; Instabilities; ISM: bubbles; ISM: structure

Indexed keywords

BACKGROUND MEDIUM; BUBBLE RADIUS; CLOSE GROUPS; COLUMN DENSITY; EFFECTIVE ENERGY; ENERGY DEPOSITIONS; ENERGY INJECTION; ENERGY RESPONSE; FEEDBACK EFFECTS; FREE PARAMETERS; GALACTIC WINDS; GALAXIES: ISM; GALAXY EVOLUTION; HYDRODYNAMIC SIMULATION; INTERNAL STRUCTURE; INTERSTELLAR MEDIUMS; ISM: BUBBLES; ISM: STRUCTURE; LOSS OF ENERGY; MASSIVE STARS; RADIATIVE COOLING; SCALE EFFECTS; SPATIAL CONFIGURATION; STELLAR WIND; SUPERNOVA EXPLOSION; THICK SHELLS; TIME-DEPENDENT; TIME-SCALES;

ENERGY EFFICIENCY; GALAXIES; HYDRODYNAMICS; IONIZING RADIATION; MERGING; STABILITY; THERMODYNAMICS; THREE DIMENSIONAL COMPUTER GRAPHICS; UNCERTAINTY ANALYSIS;

STARS;

EID: 84872904699     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220060     Document Type: Article

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