群居动物 发表于 2025-3-26 22:59:44

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厨房里面 发表于 2025-3-27 04:16:53

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Lacerate 发表于 2025-3-27 06:12:33

https://doi.org/10.1007/978-1-4419-1034-9ies and potentially to test the extent of their dark matter halos as a function of the density of the environment. Here I describe simulations of observational data and present a maximum likelihood method to infer the average properties of an ensemble of cluster galaxies.

intoxicate 发表于 2025-3-27 09:32:37

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VICT 发表于 2025-3-27 14:07:30

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小平面 发表于 2025-3-27 21:32:53

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Intercept 发表于 2025-3-28 02:01:18

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谷类 发表于 2025-3-28 05:35:08

https://doi.org/10.1007/978-3-540-85910-9henomenology of late-type galaxies in the local Universe is revised as follows: 1) M/L in the NIR is constant; 2) population I indicators, namely: the atomic hydrogen content, the current star formation rate, the luminosity and the surface brightness of the young stellar population, traced by the bl

intolerance 发表于 2025-3-28 06:29:27

Christen D. Upper,Susan S. Hirano) is adopted and model parameters are adjusted to reproduce the CM relation of Coma ellipticals. Two evolutionary sequences are calculated under the contexts of . and age ., both can equally explain the CM relation at the present epoch. The confrontation with the observational CM diagrams of E/SO ga

揉杂 发表于 2025-3-28 13:33:02

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查看完整版本: Titlebook: Galaxy Scaling Relations: Origins, Evolution and Applications; Proceedings of the E Luiz Nicolaci Costa,Alvio Renzini Conference proceeding