星际分子

星际分子HCN超精细碰撞跃迁的R矩阵传播子方法计算

The calculation of the hyperfine collision transitions for the interstellar molecule HCN by the method of R-matrix propagator

星际分子CH3CO~+与其等电子体系BH3CO的量子化学研究

A quantum chemical study on the interstellar molecule ch_3co + and its iso-electron system bh_3co

利用IOS近似模型，计算了星际分子云条件下E型CH3CN-H2含超精细能级的的碰撞跃迁速率系数。

IOS ( infinite order sudden ) approximation , the hyperfine collisional transitional rate coefficients of E-type CH3CN-H2 have been calculated under the conditions of interstellar molecular clouds .

星际分子云平均寿命的研究

A study of the mean lifetime of interstellar molecular clouds

关于星际分子的客观性的证明

The objectivity certification of interstellar molecules

星际分子正-NH3和He的超精细跃迁碰撞截面和速率系数的理论计算

Theoretical calculations of the collision cross sections and rate coefficients for the hyperfine transitions of interstellar molecular ortho-nh_3 colliding with he

目前了解的恒星形成的一个基本图象是，恒星是由一个足够大质量的星际分子气体云在其自引力作用下塌缩而形成。

The current picture is that stars are formed during the collapse of a large enough self gravitating interstellar molecular cloud .

一方面是星际分子云与恒星形成的天文研究取得了令人瞩目的成就.低温大质量星际分子云中的磁场

Major improvement has been made in the studies of interstellar molecular clouds and star formation . MAGNETIC FIELDS IN COLD AND MASSIVE CLOUDS

研究表明，包括太阳在内的恒星是由冷暗的星际分子云收缩形成的。

It has been shown that stars , including our own solar system , are formed by contraction of cold and dark interstellar clouds .

以星际分子的发现为案例，探讨了星际分子的证认与星际分子客观性的关系；

Basing on the case of the discovery of interstellar molecules , this paper discusses the relationship between the identification of interstellar molecules and the objectivity of interstellar molecules .

星际氢分子数量的取值应当比Gordon值除以1.7更小；

The value of interstellar molecular hydrogen distribution should be smaller than the Gordon 's value divided by 1.7 ;

关于气相反应形成星际氢分子机理的研究

Study about mechanism to form interstellar hydrogen molecule by gas phase reaction

星际甲醇分子脉泽的辐射抽运研究

A study of the radiative pumping of interstellar methanol Masers