摘要
Astrochemistry has made great progress in recent years.Especially the grain surface chemistry played important roles in the explanation of the formation of the interstellar molecules.In this review,we will discuss the progress,including the di erent numerical methods to simulate the ice mantles in the astrochemical models.We will also introduce the laboratory astrochemical experimental results,and their contributions to the grain surface chemistry in the review.
基金
the National Natural Science Foundation of China(No.11673054)
Xinjiang Tianchi Bairen Project.
