Detection of nonthermal emission from the bow shock of a massive runaway star

Autor: Paula Benaglia, Gustavo E. Romero, Anabella T. Araudo, C. S. Peri, Josep Martí

Publikováno v: CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP

Context. The environs of massive, early-type stars have been inspected in recent years in the search for sites where particles can be accelerated up to relativistic energies. Wind regions of massive binaries that collide have already been established

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7251ceb01872cc184923126f0646249f