New Astronomy Reviews
New Astronomy Reviews is a review journal published by Elsevier, established in 1998, covering every field of astronomy and astrophysics, with a 2025 Journal Impact Factor of 15.2《新天文学评论》是由(Elsevier)出版、1998 年创刊的天文学与天体物理综述期刊,涵盖该学科全部领域,2025 年影响因子为 15.2。
Scope
- It publishes review articles in all fields of astronomy and astrophysics, whether theoretical, observational or instrumental该刊发表天文学与天体物理全领域的理论、观测与仪器综述文章。
- It covers solar physics, planetary systems, stellar, galactic and extragalactic astronomy and astrophysics, as well as cosmology内容涵盖太阳物理、行星系统、恒星、星系与河外天文学以及宇宙学。[1]
- Review papers may span any wavelength from radio to gamma-ray综述论文可覆盖从射电到伽马射线的任意波段。[2]
- It also welcomes focus reviews, shorter papers that present only recent results from fields with important advances该刊另设焦点综述,为篇幅较短的文章,仅呈现近年取得重要进展领域的近期结果。
- Papers containing substantial new research are deemed out of scope and should be sent to regular research journals含大量新研究成果的论文不属于该刊范畴,应投向常规研究型期刊。[3]
- The journal is open to proposals on interdisciplinary and emerging topics such as astrobiology, astroparticle physics and astrochemistry该刊也欢迎天体生物学、天体粒子物理与天体化学等交叉与新兴主题的投稿提案。
History
- It was established in 1998 by Elsevier Science, continuing the series Vistas in Astronomy that ran from 1955 to 1997该刊于 1998 年创刊,接续 1955 至 1997 年间出版的(Vistas in Astronomy)。
- It is issued by Elsevier, whose headquarters are in Amsterdam in the Netherlands该刊由总部位于荷兰阿姆斯特丹的(Elsevier)出版。
- Its impact factor was 3.286 in 2021, 8.682 in 2022, 26.8 in 2024 and 15.2 in 2025其影响因子 2021 年为 3.286,2022 年为 8.682,2024 年为 26.8,2025 年为 15.2。
- It ranks fifth out of 86 journals in the JCR Astronomy and Astrophysics category, placing it in the first quartile该刊在(JCR)天文学与天体物理类别 86 种期刊中排名第五,居第一四分位。
- Its SCImago Journal Rank is 2.404 and its Source Normalized Impact per Paper is 1.504其(SCImago)期刊排名为 2.404,每篇论文归一化影响为 1.504。
- It is indexed in the Science Citation Index Expanded该刊被(Science Citation Index Expanded)收录。
Editors
- The coordinating editor is Cathie Clarke of the University of Cambridge, who researches star formation and exoplanets协调编辑为(University of Cambridge)的 Cathie Clarke,研究方向为恒星形成与系外行星。
- Editors include Jack Lissauer of NASA Ames Research Center and Marcelo Miller Bertolami of the La Plata Institute for Astrophysics编辑包括(NASA Ames Research Center)的 Jack Lissauer 与(La Plata Institute for Astrophysics)的 Marcelo Miller Bertolami。
- Other editors are Supriya Pan of Presidency University Kolkata and Gavin Rowell of the University of Adelaide其他编辑为(Presidency University Kolkata)的 Supriya Pan 与(University of Adelaide)的 Gavin Rowell。
- Advisors are Yi-Fu Cai of the University of Science and Technology of China and Ezequiel Treister of the University of Tarapaca顾问为(University of Science and Technology of China)的 Yi-Fu Cai 与(University of Tarapaca)的 Ezequiel Treister。
- The board counts seven editors and editorial board members drawn from seven countries or regions编委会共有七名编辑与编委,来自七个国家和地区。
- Papers are usually written and submitted upon the invitation of one of the editors, although proposals are also welcomed论文通常经某位编辑邀请后撰写与投稿,同时也欢迎主动提交提案。
References
- ^Perivolaropoulos L, Skara F. Challenges for Lambda CDM: An update. New Astronomy Reviews, 2022, 95: 101659. DOI: 10.1016/j.newar.2022.101659
- ^Ingram A R, Motta S E. A review of quasi-periodic oscillations from black hole X-ray binaries: Observation and theory. New Astronomy Reviews, 2019, 85: 101524. DOI: 10.1016/j.newar.2020.101524
- ^Alexander D M, Hickox R C. What drives the growth of black holes? New Astronomy Reviews, 2012, 56: 93-121. DOI: 10.1016/j.newar.2011.11.003