XMM-NewtonandChandraX-ray follow-up observations of the VHE gamma-ray source HESS J1507-622

2014/05/21 by O. Tibolla, S. Kaufmann, K. Kosack · 5 citations
Physics and Astronomy · #Aerospace engineering #Archaeology #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Context (archaeology) #Demography #Engineering physics #Gamma ray #Gamma-ray bursts and supernovae #Geography #High energy #Physics #Population #Range (aeronautics) #astro-ph.HE

paper · pdf · doi:10.1051/0004-6361/201321778

published in Astronomy and Astrophysics 567, A74 (EDP Sciences) · Accepted for publication in A&A

arxiv created 2014/05/21 · openalex publication_date 2014/05/29 · arxiv updated 2014/09/05 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The discovery of the unique source HESS J1507-622 in the very high energy (VHE) range (100 GeV−100 TeV) opened new possibilities to study the parent population of ultra-relativistic particles found in astrophysical sources and underlined the possibility of new scenarios/mechanisms crucial for understanding the underlying astrophysical processes in nonthermal sources.

Citations

• HESS J1507-622: an unique unidentified source off the Galactic Plane
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