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Monica Valluri uses numerical calculations and simulations to probe observed galactic phenomena in order to understand the physical processes that produce them. Her current focus areas are supermassive black holes (see below) and the interactions between dark matter and luminous matter in galaxies. Her analysis of simulations of dark matter halos have shown, for example, why those with gas and stars tend to be rounder. It appears that the luminous matter serves to slightly deform dark matter particles’ box-shaped orbits, resulting in a halo that is rounder than if it were comprised solely of dark matter. The implication is that the orbits of the Milky Way’s stars might serve as a probe of its dark halo’s shape.
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论文共 165 篇作者统计合作学者相似作者
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Monica Valluri,Parker Fagrelius,Sergey. E. Koposov,Ting S. Li,Oleg Y. Gnedin,Eric F. Bell, Raymond G. Carlberg,Andrew P. Cooper, Jessia N. Aguilar,Carlos Allende Prieto,Vasily Belokurov, Leandro Beraldo e Silva,
arxiv(2024)
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Namitha Kizhuprakkat,Andrew P. Cooper, Alexander H. Riley,Sergey E. Koposov,Jessica Nicole Aguilar,Steven Ahlen,Carlos Allende Prieto,David Brooks,Todd Claybaugh,Kyle Dawson, Axel de la Macorra, Peter Doel,
arxiv(2024)
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 1 (2024): 1195-1217
A. G. Adame,J. Aguilar,S. Ahlen, S. Alam, G. Aldering,D. M. Alexander, R. Alfarsy,C. Allende Prieto, M. Alvarez,O. Alves,A. Anand,F. Andrade-Oliveira,
Misty C. Bentz, Madison Markham,Sara Rosborough,Christopher A. Onken,Rachel Street,Monica Valluri,Tommaso Treu
ASTROPHYSICAL JOURNALno. 1 (2023): 25
arXiv (Cornell University) (2023)
arXiv (Cornell University) (2023)
arXiv (Cornell University) (2023)
The Astrophysical Journalno. 2 (2023): 76-76
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