Envelope expansion with core collapse - II. Quasi-spherical self-similar solutions for an isothermal magnetofluid

Monthly Notices of the Royal Astronomical Society

Volumn 364, Issue 4, 2005, Pages 1168-1184

  Yu, Cong ^a,b   Lou, Yu Qing ^c,d,e,f  

^a Chinese Academy of Sciences   (China)

^b UNIVERSITY OF CHINESE ACADEMY OF SCIENCES   (China)

^c CHINESE ACADEMY OF SCIENCES   (China)

^d TSINGHUA UNIVERSITY   (China)

^e AIX MARSEILLE UNIVERSITÉ   (France)

^f UNIVERSITY OF CHICAGO   (United States)

Author keywords

MHD; Planetary nebulae: general; Stars: AGB and post AGB; Stars: formation; Stars: winds, outflows; Waves

Indexed keywords

EXPANSION; GALAXIES; ISOTHERMS; SUPERNOVAE; TOPOLOGY;

ACCRETION RATE; CORE COLLAPSE; MAGNETIC-FIELD; MAGNETOSONIC; PLANETARY NEBULAE:GENERAL; SELF-SIMILAR; SELF-SIMILAR SOLUTION; STARS FORMATION; STARS: WINDS OUTFLOWS; STARS:AGB AND POST AGB;

MAGNETOHYDRODYNAMICS;

EID: 29144448732     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09612.x     Document Type: Article

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