메뉴 건너뛰기




Volumn 363, Issue 1828, 2005, Pages 715-724

Cooling and clusters: When is heating needed?

Author keywords

Active methods; Clusters; Cooling flows; Galaxies; Galaxy formation; Numerical methods

Indexed keywords


EID: 14844304381     PISSN: 1364503X     EISSN: None     Source Type: Journal    
DOI: 10.1098/rsta.2004.1515     Document Type: Article
Times cited : (5)

References (36)
  • 15
    • 33749006536 scopus 로고    scopus 로고
    • Galaxy evolution: Theory and observations
    • ed. V. Avila-Reese, C. Firmani, C. S. Frenk & C. Allen
    • Fabian, A. C. 2003 Galaxy evolution: theory and observations (ed. V. Avila-Reese, C. Firmani, C. S. Frenk & C. Allen). Revista Mexicana de Astronomía y Astrofíisica (Serie de Conferencias) 17, 303-313.
    • (2003) Revista Mexicana de Astronomía y Astrofíisica (Serie de Conferencias) , vol.17 , pp. 303-313
    • Fabian, A.C.1
  • 26
    • 0000612316 scopus 로고    scopus 로고
    • O'Shea, B. W., Bryan, G., Bordner, J., Norman, M. L., Abel, T., Harkness, R. & Kritsuk, A. 2004 In Adaptive Mesh Refinement - Theory and Applications. Proc. Chicago Workshop on Adaptive Mesh Refinement Methods, 3-5 September 2003 (ed. T. Plewa, T. Linde & V. G. Weirs). Springer Lecture Notes in Computational Science and Engineering, vol. 41. Pierce, F. R., Thomas, P. A., Couchman, H. M. P. & Edge, A. C. 2000 Mon. Not. R. Astr. Soc. 317, 1029.
    • (2000) Mon. Not. R. Astr. Soc. , vol.317 , pp. 1029
    • Pierce, F.R.1    Thomas, P.A.2    Couchman, H.M.P.3    Edge, A.C.4


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.