Autor:
Calderón Espinoza, Diego
Cuadra, Jorge.
Schartmann, Marc
Burkert, Andreas
Plewa, P.
Eisenhauer, F.
Habibi, M.
The source G2 has already completed its pericentre passage around Sgr A*, the supermassive black hole in the centre of our Galaxy. Although it has been monitored for 15 yr, its astrophysical nature and origin still remain unknown. In this work, we aim to test the hypothesis of G2 being the result...
Enlace original:
https://repositorio.uc.cl/handle/11534/28876
Calderón Espinoza, Diego
,
Cuadra, Jorge.
,
Schartmann, Marc
,
Burkert, Andreas
,
Plewa, P.
,
Eisenhauer, F.
,
Habibi, M.
,
[The Galactic Centre source G2 was unlikely born in any of the known massive binaries]
,
The Galactic Centre source G2 was unlikely born in any of the known massive binaries
