找回密码
 To register

QQ登录

只需一步,快速开始

扫一扫,访问微社区

Titlebook: Matter in the Universe; Ph. Jetzer,K. Pretzl,R. Steiger Book 2002 Springer Science+Business Media B.V. 2002 Big Bang.Cosmology.Dark matter

[复制链接]
楼主: 服装
发表于 2025-3-25 06:08:13 | 显示全部楼层
发表于 2025-3-25 09:11:41 | 显示全部楼层
发表于 2025-3-25 14:06:22 | 显示全部楼层
Clouds and Diffuse Baryonic Dark Matteroud suggest that at most about 20% of the halo dark matter is in form of MACHOs (Massive Astrophysical Compact Halo Objects). The dark matter could also, at least partially, be made of cold molecular clouds (mainly H.). We proposed a model for baryonic dark matter, according to which dark clusters o
发表于 2025-3-25 16:29:24 | 显示全部楼层
Mass Distribution in Our Galaxylo. A new luminosity model consistent with the COBE NIR data and the apparent magnitude distributions of bulge clump giant stars has bulge/bar length of (≃ 3.5 kpc, axis ratios of 1:(0.3–0.4):0.3, and short disk scale-length (≃ 2.1 kpc). Gas-dynamical flows in the potential of this model with consta
发表于 2025-3-25 20:09:17 | 显示全部楼层
发表于 2025-3-26 00:18:36 | 显示全部楼层
发表于 2025-3-26 07:50:16 | 显示全部楼层
Dark Quark ‘Stars’: Do They Matter for ΩMatter?and antileptons 2) a shell of hadrons in particular ., ., Λ and Σ. and leptons or antileptons and 3) a shell of hydrogen in the superfluid phase. If the superfluid hydrogen phase goes over into the electromagnetic plasma phase at densities well below one atom (10 fm)., as is usually assumed, the hyd
发表于 2025-3-26 10:39:52 | 显示全部楼层
978-90-481-6038-9Springer Science+Business Media B.V. 2002
发表于 2025-3-26 13:05:23 | 显示全部楼层
发表于 2025-3-26 17:29:10 | 显示全部楼层
 关于派博传思  派博传思旗下网站  友情链接
派博传思介绍 公司地理位置 论文服务流程 影响因子官网 SITEMAP 大讲堂 北京大学 Oxford Uni. Harvard Uni.
发展历史沿革 期刊点评 投稿经验总结 SCIENCEGARD IMPACTFACTOR 派博系数 清华大学 Yale Uni. Stanford Uni.
|Archiver|手机版|小黑屋| 派博传思国际 ( 京公网安备110108008328) GMT+8, 2025-5-18 03:04
Copyright © 2001-2015 派博传思   京公网安备110108008328 版权所有 All rights reserved
快速回复 返回顶部 返回列表