Gamma-rays and neutrinos from dense environment of massive binary systems in open clusters
arXiv:1410.7553 · doi:10.1103/PhysRevD.90.103008
Abstract
TeV gamma-ray emission has been recently observed from direction of a few open clusters containing massive stars. We consider the high energy processes occurring within massive binary systems and in their dense environment by assuming that nuclei, from the stellar winds of massive stars, are accelerated at the collision region of the stellar winds. We calculate the rates of injection of protons and neutrons from fragmentation of these nuclei in collisions with stellar radiation and matter of the winds from the massive companions in binary system. Protons and neutrons can interact with the matter, within the stellar wind cavity and within the open cluster, producing pions which decay into -rays and neutrinos. We discuss the detectability of such -ray emission by the present and future Cherenkov telescopes for the case of two binary systems Eta Carinae, within the Carina Nebula, and WR 20a, within the Westerlund 2 open cluster. We also calculate the neutrino fluxes produced by protons around the binary systems and within the open clusters. This neutrino emission is confronted with ANTARES upper limits on the neutrino fluxes from discrete sources and with the sensitivity of IceCube.
15 pages, 9 figures, accepted to Physical Review D
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Cited by in corpus (4)
- A VLT/FLAMES survey for massive binaries in Westerlund 1: VII. Cluster census
- Probing the hadronic nature of the gamma-ray emission associated with Westerlund 2
- A lepto-hadronic model of gamma rays from the Eta Carinae and prospects for neutrino telescopes
- Searching for a Galactic component in the IceCube track-like neutrino events