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Volumn 271, Issue 2, 2000, Pages 103-126

Modeling the star formation in galaxies using the chemo-dynamical SPH code

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[No Author keywords available]

Indexed keywords


EID: 0034366246     PISSN: 0004640X     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1002485702347     Document Type: Article
Times cited : (14)

References (78)
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    • Presented as a poster in the Isaac Newton Institute Workshop: June 22-27, 1998, Cambridge, U.K. (astro-ph/9807059)
    • Berczik, P.: 1998, Presented as a poster in the Isaac Newton Institute Workshop: Astrophysical Discs, June 22-27, 1998, Cambridge, U.K. (astro-ph/9807059).
    • (1998) Astrophysical Discs
    • Berczik, P.1
  • 49
    • 4243824964 scopus 로고    scopus 로고
    • submitted, (astro-ph/9801073)
    • Navarro, J.F.: 1998, Astrophys. J., submitted, (astro-ph/9801073).
    • (1998) Astrophys. J.
    • Navarro, J.F.1
  • 60
    • 4243762781 scopus 로고    scopus 로고
    • in press. Astronomical Institute University of Basel. Preprint Series No. 108
    • Samland, M.: 1997, Astrophys. J., in press. Astronomical Institute University of Basel. Preprint Series No. 108.
    • (1997) Astrophys. J.
    • Samland, M.1
  • 62
    • 84891227232 scopus 로고
    • M. Peimbert and J. Jugaku (eds.), Reidel, Dordrecht
    • Silk, J.: 1987, in: M. Peimbert and J. Jugaku (eds.), Star Forming Regions, IAU Symp. 115, Reidel, Dordrecht, pp. 557.
    • (1987) Star Forming Regions, IAU Symp. , vol.115 , pp. 557
    • Silk, J.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.