Equatorial outflows driven by jets in Population III microquasars

Binary systems of Population III can evolve to microquasars when one of the stars collapses into a black hole. When the compact object accretes matter at a rate greater than the Eddington rate, powerful jets and winds driven by strong radiation pressure should form. We investigate the structure of t...

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Detalles Bibliográficos
Autores principales:	Sotomayor Checa, Pablo Omar, Romero, Gustavo Esteban, Bosch-Ramon, Valentí
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2021
Materias:	Ciencias Astronómicas Accretion, accretion disks Stars: black holes Stars: winds, outflows Stars: Population III X-rays: binaries
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/129283
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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