Testing the nature of Sgr A* with the S-2 star orbit data

Las estrellas del cúmulo S que orbitan alrededor del centro Galáctico, proveen uno de los mejores observables astrofísicos para inferir el potencial gravitatorio generado por la fuente central Sgr A*, tradicionalmente asumida como un Agujero Negro (BH). Un modelo alternativo para Sgr A* es el de Ruf...

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Detalles Bibliográficos
Autores principales:	Crespi, Valentina, Argüelles, Carlos Raúl, Mestre, Martín Federico
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2023
Materias:	Ciencias Astronómicas Galaxy: center dark matter
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/164673
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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