1) cD galaxy-galaxies
cD星系-星系
2) cD galaxy
cD星系
1.
The peculiar velocity of the central cD galaxy is estimated as 235±72 km·s-1,indicating that the cD galaxy was formed before the complete virialization.
计算出中心cD星系的本动速度为235±72 km。
3) starburst galaxies
星暴星系
1.
The observations and studies of the OH megamasers associated with AGN and starburst galaxies are the very efficient tools to investigate characteristics of their central sources an.
对河外星系OH超脉泽的观测和研究,是探测和研究其所成协的活动星系核、星暴星系的中央源和拱核盘的有效工具。
4) quasi-stellar galaxy(QSG)
类星星系
5) stars/galaxies
恒星/星系
1.
Classification of stars/galaxies based on AutoClass
基于自动聚类算法(AutoClass)的恒星/星系分类
6) galaxy
[英]['ɡæləksi] [美]['gæləksɪ]
星系
1.
Redshift Estimation of Galaxy Spectra Based on Similarity Measure;
基于相似性度量的星系光谱红移估计
2.
The effect of the homogeneous collisionless particles of dark matter on the gravitational field of a galaxy, whose mass density will fall exponentially with radius, is considered in the linear and successive approximations.
本文用线性近似法和选代法研究均匀无碰撞暗物质粒子对质量密度按指数律下降分布的星系引力场的影响，导出了在无碰撞暗物质粒子背景下星系引力场的引力分布。
3.
Since thick disks in SO galaxies were originally detected in 1979,thick-disk compo- nents have been discovered in many disk galaxies,and there are more and more observational evidences that the thick disk in an external galaxy should be a component of the galaxy which is structurally,chemically and kinematically distinct from the thin disk of the galaxy.
自1979年以来,越来越多的观测证据表明,在许多盘状星系中普遍存在厚盘成分,它们在结构、化学组成和运动学等方面与薄盘有着明显的不同。
补充资料：互扰星系
二十世纪五十年代《帕洛马天图》问世后，兹威基等人根据星系的形态特征，认为有些星系处在引力不稳定状态，其中有的星系对、星系串或星系链彼此并非隔绝，而是在引力作用下互相干扰，破坏了星系的正常形态，甚至出现针状的、纤维状的或扫帚状的星系际桥状结构。他把这种星系对和多重星系称为互扰星系。沃龙佐夫-韦利亚米诺夫编有互扰星系图和表，载有1,800个互扰星系。
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