FLIP
发表于 2025-3-25 06:08:13
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Grandstand
发表于 2025-3-25 09:11:41
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险代理人
发表于 2025-3-25 14:06:22
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
CLOUT
发表于 2025-3-25 16:29:24
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
原来
发表于 2025-3-25 20:09:17
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时间等
发表于 2025-3-26 00:18:36
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obsession
发表于 2025-3-26 07:50:16
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
消息灵通
发表于 2025-3-26 10:39:52
978-90-481-6038-9Springer Science+Business Media B.V. 2002
Infant
发表于 2025-3-26 13:05:23
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过度
发表于 2025-3-26 17:29:10
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