HESS J1616−508: likely to be powered by PSR J1617−5055

摘要: HESS J1616 _ 508 is one of the brightest emitters in TeV sky. Recent observations with IBIS/ISGRI telescope onboard INTEGRAL spacecraft have revealed that a young, nearby and energetic pulsar, PSR J1617 5055, powerful emitter soft γ-rays 20-100 keV domain. In this paper, we present an analysis all available data from INTEGRAL, Swift, BeppoSAX XMM-Newton telescopes view to assessing most likely counterpart High Energy Stereoscopic System (HESS) source. We find energy source fuels X/y-ray emissions derived both on basis positional morphology, timing evidence energetics system. Likewise 1.2 per cent pulsar's spin-down loss needed power 0.1-10 emission also fully consistent other sources known be associated pulsars. The relative sizes very high are expected lifetimes against synchrotron Compton losses for single parent electrons emitted pulsar. no object vicinity could reasonably considered as plausible conclude there good assume J1616-508 driven by J1617-5055 which combination inverse-Compton processes combine create observed morphology broad-band energies.