Modeling W44 as a supernova remnant in a density gradient, with a partially formed dense shell and thermal conduction in the hot interior. II. The hydrodynamic models

Astrophysical Journal

Volumn 524, Issue 1 PART 1, 1999, Pages 192-212

  Shelton, R L ^a,b,c   Cox, Donald P ^a   Maciejewski, Witold ^d   Smith, Randall K ^a,b,e   Plewa, Tomasz ^f,g   Pawl, Andrew ^a   Rózyczka, Michał ^g,h  

^a University of Wisconsin Madison   (United States)

^b NASA GODDARD SPACE FLIGHT CENTER   (United States)

^c JOHNS HOPKINS UNIVERSITY   (United States)

^d MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^g NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^h UNIVERSITY OF WARSAW   (Poland)

Author keywords

Hydrodynamics; Ism: Individual (W44); ISM: Structure; Methods: Numerical radio continuum: ISM Supernova remnants

Indexed keywords

EID: 0033543930     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/307799     Document Type: Article

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