메뉴 건너뛰기




Volumn 322, Issue 3, 1997, Pages

What can we learn from the r-element distribution of CS 22892-052?

Author keywords

Nuclear reactions; Nucleosynthesis; Solar system: general; Stars: abundances; Stars: CS 22892 052

Indexed keywords


EID: 0002778829     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (22)

References (13)
  • 4
    • 0003430520 scopus 로고    scopus 로고
    • (contribution 10 Nuclei in the Cosmos IV, Notre-Dame, 1996) in press
    • Cowan J.J., Sneden C., Truran J., et al., 1997, Nucl. Phys. A (contribution 10 Nuclei in the Cosmos IV, Notre-Dame, 1996) in press
    • (1997) Nucl. Phys. A
    • Cowan, J.J.1    Sneden, C.2    Truran, J.3
  • 7
    • 3342898997 scopus 로고    scopus 로고
    • (contribution to Nuclei in the Cosmos IV, Notre-Dame, 1996) in press
    • Goriely S., 1997, Nucl. Phys A (contribution to Nuclei in the Cosmos IV, Notre-Dame, 1996) in press
    • (1997) Nucl. Phys A
    • Goriely, S.1
  • 9
    • 0000899956 scopus 로고
    • Magain P., 1995, A&A 297, 686
    • (1995) A&A , vol.297 , pp. 686
    • Magain, P.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.