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Can A Kinematically Hot and Thick Disk Form A Bar? : Role of Highly Spinning Dark Matter Halos

Fuente: arXiv

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Detalles Bibliográficos
Autor principal:	Kataria, Sandeep Kumar
Formato:	Preprint
Publicado:	2025
Materias:	Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

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