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- W1594300913 abstract "On a analyse les vitesses radiales dans l'amas Perseus en liaison avec des donnees concernant la densite projetee et les distributions des couleurs (B-V). L'amas comporte deux composantes, un cœur (15'×20') et une barre (60'×90') en projection. Le centre de l'amas coincide avec la galaxie de Seyfert NGC 1275 qui se situe au pic de la luminosite RX de l'amas. La vitesse radiale moyenne est =5240±130 km s −1 avec σ v =1220±50 km s −1 . Le rapport masse-luminosite estime dans le cas d'un amas plat vu presque par la tranche est M/L≃100 M ○. /L ○. pour H 0 =100 km s −1" @default.
- W1594300913 created "2016-06-24" @default.
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- W1594300913 date "1985-10-01" @default.
- W1594300913 modified "2023-09-28" @default.
- W1594300913 title "The structure of the Perseus cluster of galaxies." @default.
- W1594300913 hasPublicationYear "1985" @default.
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