1) O-Ne-Mg white dwarf
氧氖镁白矮星
2) C-O white dwarf
碳氧白矮星
3) white dwarf
白矮星
1.
An argument about white dwarfs between Eddington and Chandrasekhar and its inspiration;
爱丁顿、钱德拉塞卡关于白矮星的争论及其启示
2.
The recent significant progress on both the theoretical and observational researches on white dwarfs promotes the application and development of white dwarf cosmochronology.
近几年白矮星研究在理论与观测方面都取得了很大进展,这推动了白矮星宇宙纪年学的应用和发展。
3.
It also gives a general picture of their origin in the interplanetary dust of gas,their stable evolution in the stage of main-sequence and their end with White Dwarf,Neution Star and Black Hole.
描绘出了恒星在星际气体尘埃中诞生 ,在主星序阶段稳定演化 ,最后以白矮星 ,中子星或黑洞告终的一生经历轮廓。
4) White Dwarfs
白矮星
1.
A concept and basic properties about high density stars during the latter period of seellar evolution, including white dwarfs, neutron stars and black holes are discussed.
对恒星演化后期的三类高密星体（白矮星，中子星，黑洞）的基本性质和概念作了简明介绍。
5) white dwarf (star)
白矮星(天)
6) helium white dwarf
氦白矮星
补充资料：碳氧
分子式：
CAS号：
性质：见一水碳酸钠
CAS号：
性质：见一水碳酸钠
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