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Titlebook: Baryonic Dark Matter; D. Lynden-Bell,G. Gilmore Book 1990 Kluwer Academic Publishers 1990 Dark matter.Gravity.Universe.black hole.black ho

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樓主
發(fā)表于 2025-3-21 16:43:38 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
期刊全稱Baryonic Dark Matter
影響因子2023D. Lynden-Bell,G. Gilmore
視頻videohttp://file.papertrans.cn/181/180896/180896.mp4
學(xué)科分類Nato Science Series C:
圖書封面Titlebook: Baryonic Dark Matter;  D. Lynden-Bell,G. Gilmore Book 1990 Kluwer Academic Publishers 1990 Dark matter.Gravity.Universe.black hole.black ho
影響因子The visible universe is a small perturbation on the material universe. Zwicky and Sinclair Smith in the 1930s gave evidence of invisible mass in the Coma and Virgo Clusters of Galaxies. Better optical data has only served to confound their critics and the X-ray data confirms that the gravitational potentials are many times larger than those predicted on the basis of the observed stars. Dynamical analyses of individual galaxies have found that significant extra mass is needed to explain their rotational velocities. On much larger scales, tens of megaparsecs, there is suggestive evidence that there is even more mass per unit luminosity. What is this non-luminous stuff of which the universe is made‘? How much of it is there? Need there be only one kind of stuff? There are three basic possi bili ties:- all of it is ordinary (baryonic) matter, all of it is some other kind of (non-baryonic) matter, or some of it is baryonic and some is non-baryonic.
Pindex Book 1990
The information of publication is updating

書目名稱Baryonic Dark Matter影響因子(影響力)




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Index for 2.2 (System No., References),riations in dark-to-luminous mass ratio and their correlation with galaxy properties provide material for models of galaxy formation, and may indicate that at least part of the dark material is baryonic.
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發(fā)表于 2025-3-22 03:38:44 | 只看該作者
Index for 2.2 (System No., References),uce only low-mass stars. Some larger clouds, and therefore some more massive stars, can form in the central few kpc of a flow. The wider implications of the formation of dark matter in cooling flows are discussed in the context of the formation of massive galaxies.
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Systematic Properties of Rotation Curves and Dark Matter,riations in dark-to-luminous mass ratio and their correlation with galaxy properties provide material for models of galaxy formation, and may indicate that at least part of the dark material is baryonic.
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Book 1990 one kind of stuff? There are three basic possi bili ties:- all of it is ordinary (baryonic) matter, all of it is some other kind of (non-baryonic) matter, or some of it is baryonic and some is non-baryonic.
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