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Volumn 338, Issue 2, 1998, Pages 651-660

Spectral analysis of O(He)-type post-AGB stars

Author keywords

Planetary nebulae: individual: K 1 27; Stars: abundances; Stars: AGB and post AGB; Stars: evolution; Stars: individual: HS 1522+6615; Stars: individual: HS 2209+8229

Indexed keywords


EID: 0007254250     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (38)

References (44)
  • 4
    • 0001664383 scopus 로고
    • Blöcker T. 1995, A&A 299, 755
    • (1995) A&A , vol.299 , pp. 755
    • Blöcker, T.1
  • 21
    • 0009188759 scopus 로고    scopus 로고
    • eds. C.S. Jeffery, U. Heber, ASP Conference Series
    • Jeffery, C.S., Heber, U., Hill, P.W., et al. 1996, in: Hydrogen-Deficient Stars, eds. C.S. Jeffery, U. Heber, ASP Conference Series, Vol. 96, p. 471
    • (1996) Hydrogen-Deficient Stars , vol.96 , pp. 471
    • Jeffery, C.S.1    Heber, U.2    Hill, P.W.3
  • 23
    • 3943110756 scopus 로고
    • Köppen J. 1979, A&AS 35, 111
    • (1979) A&AS , vol.35 , pp. 111
    • Köppen, J.1
  • 25
    • 3142584747 scopus 로고
    • Kohoutek L. 1977, A&A 59, 137
    • (1977) A&A , vol.59 , pp. 137
    • Kohoutek, L.1
  • 39
    • 0022947839 scopus 로고
    • Crawford D.L. (ed.)
    • Tody D. 1986, in: Crawford D.L. (ed.) Proc. SPIE 627, 733
    • (1986) Proc. SPIE , vol.627 , pp. 733
    • Tody, D.1
  • 40
    • 0000573475 scopus 로고
    • Werner K. 1986, A&A 161, 177
    • (1986) A&A , vol.161 , pp. 177
    • Werner, K.1
  • 41
    • 0345498896 scopus 로고    scopus 로고
    • Werner K. 1996, ApJ 457, L39
    • (1996) ApJ , vol.457
    • Werner, K.1
  • 43
    • 0038301693 scopus 로고    scopus 로고
    • Schielicke R.E. (ed.), Astronomische Gesellschaft, Hamburg
    • Werner K., Dreizler S., Heber U., et al. 1997, in: Schielicke R.E. (ed.), Reviews in Modern Astronomy 10, Astronomische Gesellschaft, Hamburg, p. 219
    • (1997) Reviews in Modern Astronomy , vol.10 , pp. 219
    • Werner, K.1    Dreizler, S.2    Heber, U.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.