释义 |
UBV photometry AHD[yo͞o”bē-vēʹ] D.J.[ˌjuːbiːˈviː]K.K.[ˌjubiˈvi]n.(名词)- Photometry used to obtain stellar magnitudes by comparing observed magnitudes to a standard sequence of stars.紫外蓝光视觉测光法:把观察到的星星的光度和恒星的一个标准顺序相比较,用来获得星光亮度的测光法
- u(ltraviolet) u(ltraviolet)
- b(lue) b(lue)
- v(isual) v(isual)
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