The physics of proto-neutron star winds: Implications for r-process nucleosynthesis

Astrophysical Journal

Volumn 562, Issue 2 PART II, 2001, Pages 887-908

  Thompson, Todd A ^a   Burrows, Adam ^a   Meyer, Bradley S ^b  

^a UNIVERSITY OF ARIZONA   (United States)

^b CLEMSON UNIVERSITY   (United States)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: mass loss stars: neutron; Supernovae: general

Indexed keywords

EID: 0000230410     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/323861     Document Type: Article

References (5)

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5. Burris, D. L., Pilachowski, C. A., Armandroff, T. E., Sneden, C., Cowan, J. J., & Roe, H. 2000, ApJ, 544, 302