Gamma Line Radiation Emission from Stellar Winds in Orion Complex: A test for cosmic ray origin theory

Simple item page
dc.creatorNath, Biman B.
dc.creatorBiermann, Peter L.
dc.date1994-07-01
dc.date.accessioned2026-07-07T02:19:15Z
dc.date.available2026-07-07T02:19:15Z
dc.descriptionWe consider $γ$-ray emission from heavy nuclei that are accelerated in the shocks of stellar winds and are excited in interactions with the ambient matter in the Orion complex. We show that the recent detection of $γ$-ray lines in the Orion complex by COMPTEL telescope can be explained by such a scenario, assuming cosmic abundances. The scenario is consistent with recent models of cosmic ray acceleration in stellar winds of massive stars.
dc.description8 pages, plain TeX, to appear in Monthly Notices (of RAS) pink pages
dc.identifierhttps://arxiv.org/abs/astro-ph/9407001
dc.identifierhttp://arxiv.org/abs/astro-ph/9407001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9794
dc.subjectAstrophysics
dc.titleGamma Line Radiation Emission from Stellar Winds in Orion Complex: A test for cosmic ray origin theory
dc.typetext

Files

Collections

arXiv