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IceCube Search for High-energy Neutrino Emission from TeV Pulsar Wind Nebulae
Journal article   Open access

IceCube Search for High-energy Neutrino Emission from TeV Pulsar Wind Nebulae

Maryon Ahrens, Christian Bohm, Kunal Deoskar, Chad Finley, Klas Hultqvist, Matti Jansson, Erin O'Sullivan, Christian Walck and IceCube Collaboration
The Astrophysical journal, v 898(2)
2020
url
https://doi.org/10.3847/1538-4357/ab9fa0View
Published, Version of Record (VoR)Open Access (License Unspecified) Open

Abstract

Fysik Naturvetenskap Neutrino astronomy High Energy Astrophysics Natural Sciences Physical Sciences
Pulsar wind nebulae (PWNe) are the main gamma-ray emitters in the Galactic plane. They are diffuse nebulae that emit nonthermal radiation. Pulsar winds, relativistic magnetized outflows from the central star, shocked in the ambient medium produce a multiwavelength emission from the radio through gamma-rays. Although the leptonic scenario is able to explain most PWNe emission, a hadronic contribution cannot be excluded. A possible hadronic contribution to the high-energy gamma-ray emission inevitably leads to the production of neutrinos. Using 9.5 yr of all-sky IceCube data, we report results from a stacking analysis to search for neutrino emission from 35 PWNe that are high-energy gamma-ray emitters. In the absence of any significant correlation, we set upper limits on the total neutrino emission from those PWNe and constraints on hadronic spectral components.

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Collaboration types
Domestic collaboration
International collaboration
Web of Science research areas
Astronomy & Astrophysics
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