Dark Matter
天体物理学
2007-05-23 v1
摘要
Observations in the optical, in X-rays, and gravitational lensing of galaxies, clusters of galaxies, and large-scale structure are beginning to provide clues to the dark matter problem. I review the impact of these observations on some of the main questions relating to dark matter: How much dark matter is there? Where is it located? What is the nature of the dark matter? and what is the amount of baryonic dark matter.
引用
@article{arxiv.astro-ph/9611080,
title = {Dark Matter},
author = {Neta Bahcall},
journal= {arXiv preprint arXiv:astro-ph/9611080},
year = {2007}
}
备注
Figures can be obtained by e-mail to [email protected]