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Volumn 345, Issue 3, 1999, Pages 831-840

Three-dimensional simulations of classical novae

Author keywords

Convection; Hydrodynamics; Nuclear reactions, nucleosynthesis, abundances; Stars: Novae, cataclysmic variables; Stars: White dwarfs

Indexed keywords


EID: 3943096706     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (41)

References (15)
  • 5
    • 0004543767 scopus 로고
    • Müller E., 1986, A&A 162, 103
    • (1986) A&A , vol.162 , pp. 103
    • Müller, E.1
  • 8
    • 0010929078 scopus 로고
    • Bode M., Evans A. (eds.) Wiley, New York
    • Starrfield S., 1989, In: Bode M., Evans A. (eds.) The Classical Novae. Wiley, New York, p. 39
    • (1989) The Classical Novae , pp. 39
    • Starrfield, S.1
  • 9
    • 0010871640 scopus 로고
    • Sahade J., McCluskey G.E., Kondo Y. (eds.) Kluwer, Dordrecht
    • Starrfield S., 1993, In: Sahade J., McCluskey G.E., Kondo Y. (eds.) The Realm of Interacting Binary Stars. Kluwer, Dordrecht, p. 209
    • (1993) The Realm of Interacting Binary Stars , pp. 209
    • Starrfield, S.1
  • 10
    • 0010859268 scopus 로고
    • Roxburgh I., Masnou J.L. (eds.) Springer, Heidelberg
    • Starrfield S., 1995, In: Roxburgh I., Masnou J.L. (eds.) Physical Processes in Astrophysics. Springer, Heidelberg, p. 99
    • (1995) Physical Processes in Astrophysics , pp. 99
    • Starrfield, S.1
  • 13
    • 0007591384 scopus 로고
    • Barnes C.A., Clayton D.D., Schramm D.N. (eds.) Cambridge University Press, Cambridge
    • Truran J.W., 1982, In: Barnes C.A., Clayton D.D., Schramm D.N. (eds.) Essays in Nuclear Physics. Cambridge University Press, Cambridge, p. 467
    • (1982) Essays in Nuclear Physics , pp. 467
    • Truran, J.W.1
  • 14
    • 0010919228 scopus 로고
    • Cassatella A., Viotti R. (eds.) Springer, Heidelberg
    • Truran J.W., 1990, In: Cassatella A., Viotti R. (eds.) The Physics of Classical Novae. Springer, Heidelberg, p. 373
    • (1990) The Physics of Classical Novae , pp. 373
    • Truran, J.W.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.