Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters-Reference-Cited by-同舟云学术

Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters

Author:

Laganá T F¹,Durret F²,Lopes P A A³^ORCID

Affiliation:

1. NAT, Universidade Cruzeiro do Sul, Rua Galvão Bueno, 868, CEP 01506-000, Sao Paulo, SP, Brazil

2. Sorbonne Université, CNRS, UMR 7095, Institut d’Astrophysique de Paris, 98bis Bd Arago, F-75014 Paris, France

3. Observatório do Valongo, Universidade Federal do Rio de Janeiro, Ladeira do Pedro Antônio 43, Rio de Janeiro, RJ 20080-090, Brazil

Funder

Fundação de Amparo à Pesquisa do Estado de São Paulo

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Centre National d’Etudes Spatiales

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference126 articles.

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