Main Image
Volume 354 - High Energy Phenomena in Relativistic Outflows VII (HEPRO VII) - Relativistic outflows from galactic sources
GRS 1758-258 as a winged microquasar
J. Martí,* P.L. Luque-Escamilla, J.M. Paredes, V. Bosch-Ramon
*corresponding author
Full text: pdf
Published on: 2020 February 25
Abstract
A deep radio image of the microquasar GRS 1758-258 has evidenced for the first time a new link with the so called `winged' radio galaxies. This opens a new perspective for the understanding of these secondary lobe features in relativistic jets. The fact that we also find them in a relativistic stellar outflow is better understood in the context of hydrodynamic models. This is in contrast to other alternative interpretations that are mostly based on the spin-flip of the central black hole in radio galaxies.
DOI: https://doi.org/10.22323/1.354.0065
Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.