Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6847
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dc.contributor.authorGupta, Nayantara-
dc.contributor.authorRazzaque, Soebur-
dc.date.accessioned2018-03-06T12:15:27Z-
dc.date.available2018-03-06T12:15:27Z-
dc.date.issued2017-12-
dc.identifier.citationPhysical Review D, 2017, Vol.96, p 123017en_US
dc.identifier.issn2470-0010-
dc.identifier.issn2470-0029 (online)-
dc.identifier.urihttp://hdl.handle.net/2289/6847-
dc.descriptionOpen Accessen_US
dc.description.abstractThe stellar binary η Carinae has been observed during its full orbital period in gamma rays by the Fermi-Large Area Telescope (LAT). The shock-accelerated electrons in the colliding winds of the two stars radiate synchrotron photons in the magnetic field of the shocked region and inverse Compton photons, where the target photons are from the thermal emissions by the more massive and luminous of the two stars. The inverse Compton emission dominates the gamma-ray flux data from the η Carinae, however the spectral energy distribution shows signature of a hadronic component in the ∼10–300  GeV range during the periastron passage. Current and future air Cherenkov telescopes will be able to constrain this component at TeV energies. Acceleration of cosmic-ray protons to ≫1  TeV energies in the colliding winds, required to explain the hadronic emission component through photopion interactions, can lead to detectable signal of ≳10  TeV neutrino events in large kilometer scale neutrino telescopes.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.relation.urihttp://adsabs.harvard.edu/abs/2017PhRvD..96l3017Gen_US
dc.relation.urihttp://arxiv.org/abs/1706.10051en_US
dc.relation.urihttp://dx.doi.org/10.1103/PhysRevD.96.123017en_US
dc.rights2017 American Physical Societyen_US
dc.titleLepto-hadronic model of gamma rays from Eta Carinae and prospects for neutrino telescopes.en_US
dc.typeArticleen_US
Appears in Collections:Research Papers (A&A)

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