星际分子指存在于星际空间的无机分子和有机分子。已发现50余种星际分子，其中大多数是由碳、氢、氧、氮组成的有机分子。
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.
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。
Major improvement has been made in the studies of interstellar molecular clouds and star formation.
星际分子、星际微波激射、太阳引力弯曲的检验都与射电干涉仪紧密联系。
The test of interstellar molecules, interstellar maser and solar gravitational deflection are closely related to radio interferometer.
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