Astronomy and Astrophysics Review
Published by Springer Nature
ISSN : 0935-4956 eISSN : 1432-0754
Abbreviation : Astron. Astrophys. Rev.
Aims & Scope
The Astronomy and Astrophysics Review is devoted to all areas of astronomy and astrophysics, including subjects bordering on other fields.
Thus developments in laboratory or particle physics directly relevant to astronomy may be included, as well as cosmic ray physics, studies in the solar system, astrobiology, instrumentation and computational and statistical methods with specific astronomical applications.
It is intended that all important fields be reviewed from time to time, whereby the frequency of review will be dependent on the amount of activity in the different areas.
The journal emphasizes review articles that are not only of the highest quality in their scientific content, but also have a good readability.
They thereby provide an excellent starting point for scientists or students seeking access to a new or unfamiliar field as well as for researchers and lecturers in need of authoritative material in fields with which they are less familiar.
View Aims & ScopeMetrics & Ranking
Impact Factor
Year | Value |
---|---|
2025 | 26.5 |
2024 | 27.80 |
Journal Rank
Year | Value |
---|---|
2024 | 94 |
Journal Citation Indicator
Year | Value |
---|---|
2024 | 640 |
SJR (SCImago Journal Rank)
Year | Value |
---|---|
2024 | 9.465 |
Quartile
Year | Value |
---|---|
2024 | Q1 |
Impact Factor Trend
Abstracting & Indexing
Journal is indexed in leading academic databases, ensuring global visibility and accessibility of our peer-reviewed research.
Subjects & Keywords
Journal’s research areas, covering key disciplines and specialized sub-topics in Earth and Planetary Sciences and Physics and Astronomy, designed to support cutting-edge academic discovery.
Most Cited Articles
The Most Cited Articles section features the journal's most impactful research, based on citation counts. These articles have been referenced frequently by other researchers, indicating their significant contribution to their respective fields.
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Accurate masses and radii of normal stars: modern results and applications
Citation: 1208
Authors: G., J., A.
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Modelling the behaviour of accretion flows in X-ray binaries
Citation: 1056
Authors: Chris, Marek, Aya
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Common envelope evolution: where we stand and how we can move forward
Citation: 819
Authors: N., S., X., O., C. L., E., H., E., Z., X.-D., G., T., P., A., N., R., T. M., E. P. J., R. F.
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Cosmological magnetic fields: their generation, evolution and observation
Citation: 638
Authors: Ruth, Andrii
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The strongest cosmic magnets: soft gamma-ray repeaters and anomalous X-ray pulsars
Citation: 567
Authors: Sandro
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Clusters of galaxies: observational properties of the diffuse radio emission
Citation: 554
Authors: Luigina, Gabriele, Federica, Matteo