1) emission line
发射线
1.
Associating with structure of disk in the outer region, we discuss the properties of emission line 1n the disk.
考虑了自引力的作用，计算出了稳定的磁粘滞自引力薄吸积盘外区的结构，综合盘外区的结构，讨论了吸积盘外区的辐射性质以及发射线的有关问题。
2.
The redshifts of emission lines range from 0 to 4.
全部类星体发射线范围是从0到4。
3.
Narrow emission lines from Active Galactic Nuclei (AGNs) are produced bygas photoionized by AGN continuum on scales of pc to 10~2 pc scales.
活动星系核(AGN)的窄发射线为pc到100pc尺度上的气体被AGN的连续谱光致电离产生。
2) emission lines
发射线
1.
We used 12 moderately resolved quasar pairs from the Sloan Digitized Sky Survey(SDSS) for the study,where the equivalent widths of the Lyman-α emission lines of the foreground quasars are available in literature.
通过探究类星体对的Lyman-α的吸收线和发射线的等值宽度,研究了它们之间可能存在的相互关系。
2.
This correlation was explored in QSOs for other broad emission lines, such as Lyα, SII V1400, O VI 1034, NV 1240, Mg II 2800, Hβ4861; for narrow emission lines, such as [O III] 5007, [O II] 3727, [N v] 3426, [N III]3869; even for the Fe Kαemission line in X-ray spectrum.
Baldwin效应(Baldwin effect)指类星体(QSOs)CⅣ1549(?)发射线等值宽度(EW)与其附近连续谱光度(即发射线光度与电离连续谱光度)之间的反相关关系。
4) X-ray emission
X射线发射
1.
Investigation on Kα X-ray emission from ultraintense laser-produced hot electrons;
超强激光超热电子激发的Kα X射线发射研究
2.
The X-ray emission from the highly charged Ar 17+ ion interacting with Mo surface are measured on the 14.
观测了低速 (小于Bohr速度 )高电荷Ar17+离子与金属Mo表面相互作用的X射线发射 ,以及ArKα ,KβX射线强度随入射离子动能的变化 。
5) gamma-ray emission
γ射线发射
6) ray shooting method
射线发射法
补充资料：初级发射线谱分析
分子式：
分子量：
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性质：见X射线谱分析。
分子量：
CAS号：
性质：见X射线谱分析。
说明：补充资料仅用于学习参考，请勿用于其它任何用途。
参考词条