ASTROPHYSICS AND SPACE SCIENCE
ASTROPHYSICS AND SPACE SCIENCE(英文缩写 ASTROPHYS SPACE SCI),ISSN 0004-640X,eISSN 1572-946X 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：2025-09-21 至 2026-09-21，按本站收录文献的发表日期统计。
指标来源：jcr_cas_ifqb
期刊简介
暂无简介。
历年影响因子趋势
| JCR 数据年份 | 影响因子 | JCR 分区 |
|---|---|---|
| 2021 | 1.909 | Q3 |
| 2022 | 1.900 | Q3 |
| 2023 | 1.800 | Q3 |
| 2024 | 1.500 | Q3 |
| 2025 | 2.100 | Q3 |
ASTROPHYSICS AND SPACE SCIENCE 最新收录文献
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1. Insights into the diversity of exoplanet atmospheres in the era of JWST.
PMID:作者:日期:2026-01-01From religion to science, the quest to understand our place in the universe is one of the fundamental drivers of human progress. Since the discovery of the first exoplanet around a main sequence star in the mid-1990s, our current count of exoplanetary systems has exploded to several thousands. We ha…
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2. Prospects and challenges in developing the next generation astronomical sub-millimetre and terahertz heterodyne receivers.
PMID:作者:日期:2026-01-01The development of next-generation astronomical receivers operating at millimetre (mm), sub-mm, and terahertz frequencies is essential to meet the increasing demand for wide-field, high-spectral-resolution observations. In this work, we examine the prospects and challenges associated with advancing …
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3. Imaging black holes: a VLBI success story.
PMID:作者:日期:2026-01-01Advances in Very Long Baseline Interferometry (VLBI) have enabled, for the first time, horizon-scale images of the two most accessible supermassive black hole candidates: M87* at the centre of the elliptical galaxy Messier 87 and Sgr A* at the centre of the Milky Way. These images reveal ring-like e…
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4. The abundances of carbon and nitrogen in the atmospheres of classical Be stars.
PMID:作者:日期:2026-01-01Hot stars born as rapid rotators are expected to induce meridional currents that mix hydrogen from the envelope into the core and return CNO-cycle processed material to the envelope, which should enhance the N at the surface at the expense of C and possibly also O depending on the ambient conditions…
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5. Superluminous supernovae: diverse rise times explain diverse spectra.
PMID:作者:日期:2026-01-01Type I superluminous supernovae (SLSNe) are a diverse class of exceptionally bright massive star explosions, which typically exhibit absorption from ionised oxygen in their early spectra. While their photometric properties (luminosity and duration) both span an order of magnitude, population studies…
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6. A decade of sub-arcsecond imaging with the International LOFAR Telescope.
PMID:作者:日期:2025-01-01The International LOFAR Telescope (ILT) is a pan-European radio interferometer with baselines up to 2000 km. This provides sub-arcsecond resolution at frequencies of <200 MHz. Since starting science operations in 2012, the ILT has carried out observations for the state-of-the-art LOFAR Two-metre Sky…
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7. The spectral evolution of white dwarfs: where do we stand?
PMID:作者:日期:2024-01-01White dwarfs are the dense, burnt-out remnants of the vast majority of stars, condemned to cool over billions of years as they steadily radiate away their residual thermal energy. To first order, their atmosphere is expected to be made purely of hydrogen due to the efficient gravitational settling o…
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8. Revealing the atmospheres of highly irradiated exoplanets: from ultra-hot Jupiters to rocky worlds.
PMID:作者:日期:2023-01-01Spectroscopy of transiting exoplanets has revealed a wealth of information about their atmospheric compositions and thermal structures. In particular, studies of highly irradiated exoplanets at temperatures much higher than those found in our solar system have provided detailed information on planet…
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9. How deterministic is the Earth ionosphere's response to solar activity?
PMID:作者:日期:2022-01-01This contribution is aimed at an analysis of the dynamics of free-electron density fluctuations in the ionospheric critical plasma frequency f0F2 by using some tools from the theory of nonlinear dynamical systems. The results suggest the existence of low-dimensional attractors that point to a charac…
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10. The mystery of unidentified infrared emission bands.
PMID:作者:日期:2022-01-01A family of unidentified infrared emission (UIE) bands has been observed throughout the Universe. The current observed spectral properties of the UIE bands are summarized. These properties are discussed in the frameworks of different models of the chemical carriers of these bands. The UIE carriers r…