The enigmatic G2 cloud just passed pericentre around the Galactic Centre super-massive black hole, Sgr A. Despite all theoretical and observational efforts, its nature remains unclear. If purely gaseous, it is possible to explain it as a gas clump formed in a colliding wind binary. Here we study the hypothesis of G2 being one of such clumps ejected from the massive binary IRS 16SW....
Registro Sencillo
Registro Completo
Autor | Calderón Espinoza, Diego Nicolás Cuadra, Jorge |
Título | A massive binary system can feed Sgr A* |
Revista | Revista Mexicana de Astronomia y Astrofisica Conference Series |
Fecha de publicación | 2017 |
Resumen | The enigmatic G2 cloud just passed pericentre around the Galactic Centre super-massive black hole, Sgr A. Despite all theoretical and observational efforts, its nature remains unclear. If purely gaseous, it is possible to explain it as a gas clump formed in a colliding wind binary. Here we study the hypothesis of G2 being one of such clumps ejected from the massive binary IRS 16SW.... |
Derechos | acceso restringido |
Enlace | https://repositorio.uc.cl/handle/11534/28688 https://ui.adsabs.harvard.edu/abs/2017RMxAC..49..101C/abstract |
Materia | Galaxia Galaxias - Evolución Agujeros negros |
Se encuentra en | Latin American Regional IAU Meeting Cartagena 2016 (15o. : 2016 : Cartajena de Indias, Colombia) |
Temática | Astronomía |
Tipo de documento | comunicación de congreso |