A microquasar shot out from its birth place

• Autor(a) principal: Mirabel, I. Felix
• Data de Publicação: 2004
• Outros Autores: Rodrigues, Irapuan, Liu, Q. Z.
• Tipo de documento: Artigo
• Idioma: eng
• Título da fonte: Repositório Institucional da UFRGS
• Texto Completo: http://hdl.handle.net/10183/98761
• topic: Formacao de estrelas; Buracos negros; Estrelas de neutrons; Massa estelar; Movimento estelar; Momento linear; Supernova; Aglomerados estelares; Stars: individual: LS I +61° 303, 2CG 135+01, 3EG J0241+6103; X-rays: binaries: stars; Gamma-rays: observations; Gamma-rays: theory

We show that the microquasar LS I +61° 303 is running away from its birth place in a young complex of massive stars. The supernova explosion that formed the compact object shot out the X-ray binary with a linear momentum of 430 ± 140 Mѳ km sˉ¹, which is comparable to the linear momenta found in solitary runaway neutron stars and millisecond pulsars. The properties of the binary system and its runaway motion of 27±6 km sˉ¹ imply that the natal supernova was asymmetric and that the upper limit for the mass that could have been suddenly ejected in the explosion is ~2 Mѳ. The initial mass of the progenitor star of the compact object that is inferred depends on whether the formation of massive stars in the parent stellar cluster was coeval or a sequential process.