厚颜 发表于 2025-3-28 17:42:46
http://reply.papertrans.cn/67/6624/662323/662323_41.pngBernstein-test 发表于 2025-3-28 18:44:25
http://reply.papertrans.cn/67/6624/662323/662323_42.pngInstrumental 发表于 2025-3-29 01:24:17
http://reply.papertrans.cn/67/6624/662323/662323_43.pngcritique 发表于 2025-3-29 03:41:38
http://reply.papertrans.cn/67/6624/662323/662323_44.pngANNUL 发表于 2025-3-29 08:05:35
http://reply.papertrans.cn/67/6624/662323/662323_45.pngCLASH 发表于 2025-3-29 12:53:38
Dwarf Galaxies and Dark Matterarticles orbiting our Galaxy, their Galactocentric radial velocities and distances can be used to constrain the distribution of dark matter in the Galactic halo. Although this problem has been investigated several times in the past , there are at least two motivations for another look: (i)阻塞 发表于 2025-3-29 18:45:25
http://reply.papertrans.cn/67/6624/662323/662323_47.png向外才掩饰 发表于 2025-3-29 20:39:03
The Stellar Population at the Galactic Centerrmation in other galactic nuclei but also as an example of star formation in a bulge environment. The star formation process in the deep gravitational potential well at the center of a galaxy may well differ from that process in the less extreme circumstances found in a disk.彩色 发表于 2025-3-30 02:56:31
http://reply.papertrans.cn/67/6624/662323/662323_49.png侵略 发表于 2025-3-30 07:38:24
Hot Coronae Around Early Type Galaxies the stars of a bright elliptical galaxy would shed ~5×10... of gas. Over the last 25 years, limits on various forms of gas in early type galaxies became increasingly stringent. Models for a galactic wind, like that of MATHEWS and BAKER , were developed to explain the absence of gas. However NORM