Annual Review of Astronomy and Astrophysics天文学与天体物理学年度评论
Annual Review of Astronomy and Astrophysics(英文缩写 ANNU REV ASTRON ASTR),ISSN 0066-4146,eISSN 1545-4282,中文译名:天文学与天体物理学年度评论 是一本学术期刊。本页汇总该期刊的最新影响因子、分区信息以及最新收录于 PubMed 的文献,帮助您快速了解期刊全貌。
发文量统计区间：2025-11-01 至 2026-10-31，按本站收录文献的发表日期统计。
期刊介绍
历年影响因子趋势
| JCR 数据年份 | 影响因子 | JCR 分区 |
|---|---|---|
| 2021 | 37.226 | Q1 |
| 2022 | 33.300 | Q1 |
| 2023 | 26.300 | Q1 |
| 2024 | 32.500 | Q1 |
| 2025 | 37.300 | Q1 |
Annual Review of Astronomy and Astrophysics 最新收录文献
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1. Chemical evolution of star-forming regions.
1. 恒星形成区的化学演化PMID:日期:1998Recent advances in the understanding of the chemical processes that occur during all stages of the formation of stars, from the collapse of molecular clouds to the assemblage of icy planetesimals in protoplanetary accretion disks, are reviewed. Observational studies of the circumstellar material within 100-10,000 AU of the young star with (sub)millimeter single-dish telescopes, millimeter interferometers, and ground-based as well as space-borne infrared observatories have only become possible within the past few years. Results are compared with detailed chemical models that emphasize the coupling of gas-phase and grain-surface chemistry. Molecules that are particularly sensitive to different routes of formation and that may be useful in distinguishing between a variety of environments and histories are outlined. In the cold, low-density prestellar cores, radicals and long unsaturated carbon chains are enhanced. During the cold collapse phase, most species freeze out onto the grains in the high-density inner region. Once young stars ignite, their surroundings are heated through radiation and/or shocks, whereupon new chemical characteristics appear. Evaporation of ices drives a ''hot core'' chemistry rich in organic molecules, whereas shocks propagating through the dense envelope release both refractory and volatile grain material, resulting in prominent SiO, OH, and H2O emission. The role of future instrumentation in further developing these chemical and temporal diagnostics is discussed.