Formation and Evolution of X--ray Filaments between Galaxy Clusters
, 2000 High-resolution cosmological hydrodynamical simulations are used for studying the evolution and the properties of the gas contained in the filamentary structure connecting galaxy ...
PANTANO, ORNELLA, C. GHELLER
core
Galaxy Evolution with Manifold Learning. [PDF]
Entropy (Basel)Takeuchi TT, Cooray S, Kano RR.
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A Discrete Informational Framework for Classical Gravity: Ledger Foundations and Galaxy Rotation Curve Constraints. [PDF]
Entropy (Basel)Simons M, Allahyarov E, Washburn J.
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Unsupervised multimodal deep learning for galaxy morphology taxonomy: integrating ConvNeXtEmbeddings and morphological parameters for scalable survey science. [PDF]
Sci RepSelim IM +3 more
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Simulations of multi-phase gas in and around galaxies. [PDF]
Living Rev Comput AstrophysGronke M, E Schneider E.
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Early Type Galaxies And Reliable Galaxy Cluster Selection
, 2010 In an era of precision cosmology, clusters of galaxies are the natural consequences under the hierarchical scenario, within which clusters directly encapsulate the history of structure formation.
Song, Jeeseon
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The era of precision cosmology with voids. [PDF]
Astron Astrophys RevContarini S, Verza G, Pisani A.
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Ten common misconceptions about Galaxy (and why they are wrong!). [PDF]
PLoS Comput BiolBacon WA +10 more
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ON THE SPIRAL STRUCTURE OF DISK GALAXIES
The Astrophysical Journal, 1964 C. C. Lin, Frank H. Shu
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Community-curated Galaxy interfaces with the Galaxy Labs Engine. [PDF]
GigascienceHyde CJ +6 more
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