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Volumn 927, Issue , 2001, Pages 54-69

Non-gaussianity versus nonlinearity of cosmological perturbations

Author keywords

Clusters; Cosmic microwave background; Cosmology: large scale structure; Galaxies

Indexed keywords

ASTRONOMY; CLUSTER ANALYSIS; CONFERENCE PAPER; COSMOS; FOURIER TRANSFORMATION; GRAVITY; PARTICLE SIZE; PHYSICS; THEORY;

EID: 0034994106     PISSN: 00778923     EISSN: None     Source Type: Book Series    
DOI: 10.1111/j.1749-6632.2001.tb05621.x     Document Type: Conference Paper
Times cited : (3)

References (27)
  • 6
    • 0000922450 scopus 로고
    • Gravity, bias, and the galaxy three-point correlation function
    • (1994) Phys. Rev. Lett. , vol.73 , Issue.2 , pp. 215-219
    • Fry, N.J.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.