Abstract
We show that the microquasar LSI+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 M⊙ km s-1, 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 s-1 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 M⊙. 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.
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CITATION STYLE
Mirabel, I. F., Rodrigues, I., & Liu, Q. Z. (2004). A microquasar shot out from its birth place. Astronomy and Astrophysics, 422(2). https://doi.org/10.1051/0004-6361:200400016
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