Galaxies: a perspective from its origins

Authors

DOI:

https://doi.org/10.47456/Cad.Astro.v5n1.43825

Keywords:

galaxies, simulation, fusion

Abstract

This short article aims at setting relevant properties of galaxies in the light of recent studies. By putting particular emphasis on their formation and evolution, key issues such as the importance of accretion, dark matter, and feedback astrophysical process are briefly discussed.

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Author Biography

Diego Garcia Lambas, National University of Córdoba

Diego Garcia Lambas (diego.garcia.lambas@unc.edu.ar) é professor e pesquisador do CONICET na Universidad Nacional de Córdoba, Argentina. Foi também diretor do Observatório Astronômico de Córdoba e do Instituto de Astronomia Teórica e Experimental, IATE.

References

[1] E. Hubble, Effects of red shifts on the distribution of nebulae, The Astrophysical Journal 84, 517 (1936). DOI: https://doi.org/10.1086/143782

[2] A. Helmi, Streams, substructures and the early history of the Milky Way, Annual Re

view of Astronomy and Astrophysics 58(1), 205 (2020). DOI: https://doi.org/10.1146/annurev-astro-032620-021917

[3] H. Mo, F. van den Bosch e S. White, Galaxy Formation and Evolution (Cambridge University Press, Cambridge, 2010). DOI: https://doi.org/10.1017/CBO9780511807244

[4] M. Vogelsberger et al., Properties of galaxies reproduced by a hydrodynamic simulation, Nature 509(7499), 177 (2014). DOI: https://doi.org/10.1038/nature13316

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Published

15-03-2024

How to Cite

[1]
D. G. Lambas, “Galaxies: a perspective from its origins”, Cad. Astro., vol. 5, no. 1, pp. 102–106, Mar. 2024.

Issue

Vol. 5 No. 1 (2024): Galáxias

Section

Seção Temática

License

Copyright (c) 2024 Diego Garcia Lambas

Creative Commons License

This work is licensed under a Creative Commons Attribution 4.0 International License.