方法证据记录
Rotation Curve Analysis
Galaxy rotation curve analysis is the technique of measuring how orbital velocities change with distance from the center of a galaxy. Pioneered by Vera Rubin and W. Kent Ford Jr. in 1970, rotation curves revealed one of astronomy's great mysteries: galaxies rotate too fast to be held together by their visible stars alone, providing direct evidence for dark matter.
源记录
引文逐字复制自方法源记录。这些引文不代表任何层级的验证。
Galaxy Rotation Curve Analysis for Dark Matter Detection
分类方法记录 · process-pipeline / astronomy
- Vera C. Rubin & W. Kent Ford Jr. (1970). Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission Regions. Astrophysical Journal, 159, 379-403. · DOI 10.1086/150317
- Flores, R. A., & Primack, J. R. (1994). Structure and dynamics of galactic dark matter halos. Astrophysical Journal Letters, 427(1), L1-L4. · URL
- Sofue, Y., Tutui, Y., Honma, M., et al. (2001). Central and dark matter rotation curves of spiral galaxies. Astrophysical Journal, 547(2), 712-726. · URL
精选声明
声明已持久化到证据分类账中，每个声明都有自己的评估。
尚无精选声明
当分类账中没有声明时，此视图不会自行创建声明评估。
相关方法
从方法图中生成，显示为机器建议的关系 — 不推断任何证据声明。