On the Dark Matter Column Density in Haloes
- Авторы: Del Popolo A.1,2,3, Lee X.1
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Учреждения:
- Institute of Modern Physics
- Dipartimento di Fisica e Astronomia
- INFN, sezione di Catania
- Выпуск: Том 61, № 12 (2017)
- Страницы: 1003-1014
- Раздел: Article
- URL: https://journals.rcsi.science/1063-7729/article/view/191274
- DOI: https://doi.org/10.1134/S1063772917120022
- ID: 191274
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Аннотация
We study the correlation between the central surface density and the halo core radius of the dark matter haloes of galaxies and clusters of galaxies. We find that the surface density within the halo characteristic radius r* is not an universal quantity as claimed by some authors (e.g., [1]), but it correlates with several physical quantities (e.g., the halo mass M200 and the magnitude MB). The slope of the surface density—mass relation is 0.18 ± 0.05, leaving small room to the possibility of a constant surface density. Finally, we compare the results with the MOND prediction.
Об авторах
A. Del Popolo
Institute of Modern Physics; Dipartimento di Fisica e Astronomia; INFN, sezione di Catania
Автор, ответственный за переписку.
Email: adelpopolo@oact.inaf.it
Китай, Lanzhou; Catania; Catania
Xi-Guo Lee
Institute of Modern Physics
Email: adelpopolo@oact.inaf.it
Китай, Lanzhou
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