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Dwarf Galaxies in Focus: A Survey of Observational and Theoretical Studies

Komiljon TillaboevDepartment of Nuclear Physics and Astronomy, National University of Uzbekistan named after Mirzo Ulugbek, 4 University Str., Tashkent 100714, UzbekistanIkram TadjibaevDepartment of Applied Sciences in Primary Education, Chirchik State Pedagogical University, 104 A. Temur Str., Chirchik 111700, UzbekistanKamolidin MamadaliyevDepartment of Applied Sciences in Primary Education, Chirchik State Pedagogical University, 104 A. Temur Str., Chirchik 111700, UzbekistanDildor OtajonovaDepartment of Applied Sciences in Primary Education, Chirchik State Pedagogical University, 104 A. Temur Str., Chirchik 111700, UzbekistanMalokhat AtajonovaDepartment of Translation Theory and Practice, Urgench State University, 14 Khamid Alimjan Str., Urgench 200100, UzbekistanB. I. AbdullayevAndijan State Institute of Foreign Languages, 5 Bobirshokh Str., Andijan 170100, Uzbekistan
Galaxiesjournal2025en
ABI

Аннотация

This paper presents provides a comprehensive survey of dwarf galaxies, which represent the most numerous and diverse systems in the Universe. We discuss their definitions and morphological classifications, emphasizing the unique properties that distinguish them from globular clusters and giant galaxies. Special attention is given to their formation and evolutionary processes in the framework of hierarchical structure formation and ΛCDM cosmology, including the role of environmental mechanisms and stellar feedback. Star formation histories are explored based on observations and simulations, highlighting both bursty and extended activity across different dwarf types. We further examine the crucial role of dark matter in shaping the dynamics and structure of dwarf galaxies, as well as the core–cusp and missing satellites problems. Finally, we summarize insights from numerical simulations and theoretical models, which provide a bridge between observations and cosmological predictions. This synthesis demonstrates that dwarf galaxies remain essential laboratories for testing galaxy formation theories and probing the nature of dark matter.

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