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Astrophysics > High Energy Astrophysical Phenomena

arXiv:1301.6824 (astro-ph)
[Submitted on 29 Jan 2013 (v1), last revised 1 Feb 2013 (this version, v2)]

Title:Exploration of Galactic γ-Ray Supernova Remnants

Authors:Wenwu Tian, Jianli Zhang
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Abstract:New generational very-high-energy telescope arrays have been detecting more than 120 TeV {\gamma}-ray sources. Multi-wavelength observations on these Gamma-ray sources have proven to be robust in shedding light on their nature. The coming radio telescope arrays like ASKAP and FAST may find more faint (extended) radio sources due to their better sensitivities and resolutions, might identify more previously un-identified {\gamma}-ray sources and set many new targets for future deep surveys by very-high-energy ground-based telescopes like LHAASO. We in the paper summarize a list of known Galactic {\gamma}-ray Supernova Remnants (SNRs) with or without radio emissions so far, which includes some SNRs deserving top priority for future multi-wavelength observations.
Comments: 24 pages, 3 figures, 2 tables, Accepted by SCIENCE CHINA Physics, Mechanics & Astronomy. Background is changed, no changes in figures and tables
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE); Astrophysics of Galaxies (astro-ph.GA)
Cite as: arXiv:1301.6824 [astro-ph.HE]
  (or arXiv:1301.6824v2 [astro-ph.HE] for this version)
  https://doi.org/10.48550/arXiv.1301.6824

Submission history

From: JianLi Zhang J. L. Zhang [view email]
[v1] Tue, 29 Jan 2013 03:25:43 UTC (482 KB)
[v2] Fri, 1 Feb 2013 02:49:27 UTC (466 KB)
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