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2004ApJ...601L..75T - Astrophys. J., 601, L75-L78 (2004/January-3)
High-energy gamma rays from stellar associations.
TORRES D.F., DOMINGO-SANTAMARIA E. and ROMERO G.E.
Abstract (from CDS):
It is proposed that TeV γ-rays and neutrinos can be produced by cosmic rays (CRs) through hadronic interactions in the innermost parts of the winds of massive O and B stars. Convection prevents low-energy particles from penetrating into the wind, leading to an absence of MeV-GeV counterparts. It is argued that groups of stars located close to the CR acceleration sites in OB stellar associations may be detectable by ground-based Cerenkov telescopes.
Abstract Copyright: ∼
Journal keyword(s): Gamma Rays: Observations - Gamma Rays: Theory - Stars: Early-Type
CDS comments: Parag. 5 : TeV J2032+4131 = NAME TeV J2032+4131
Simbad objects: 5
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