In a hot bubble: Why does superbubble feedback work, but isolated supernovae do not?

Monthly Notices of the Royal Astronomical Society

Volumn 443, Issue 4, 2014, Pages 3463-3476

  Sharma, Prateek ^a   Roy, Arpita ^a,b   Nath, Biman B ^b   Shchekinov, Yuri ^c  

^a INDIAN INSTITUTE OF SCIENCE   (India)

^b RAMAN RESEARCH INSTITUTE   (India)

^c SOUTHERN FEDERAL UNIVERSITY   (Russian Federation)

Author keywords

Galaxies: ISM; ISM: bubbles; ISM: supernova remnants; Shock waves

Indexed keywords

NUMERICAL METHODS; SUPERNOVAE;

CONTINUOUS ENERGY; ENERGY INJECTION; EULERIAN HYDRODYNAMICS; GALAXIES: ISM; HYDRODYNAMIC SIMULATION; ISM: BUBBLE; ISM: SUPERNOVA REMNANTS; MECHANICAL ENERGIES; ONE-DIMENSIONAL; SHOCK-WAVES;

SHOCK WAVES;

EID: 84907359671     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stu1307     Document Type: Article

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