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    Discovery of variable VHE γ-ray emission from the binary system 1FGL J1018.6-5856 

    Abramowski, A.; Böttcher, M.; Davids, I.D.; Ivascenko, A.; Krüger, P.P.; Pekeur, N.W.; Seyffert, A.S.; Spanier, F.; Sushch, I.; Van der Walt, J.; Venter, C. (EDP Sciences, 2015)
    Re-observations with the HESS telescope array of the very high-energy (VHE) source HESS J1018–589 A that is coincident with the Fermi-LAT γ-ray binary 1FGL J1018.6–5856 have resulted in a source detection significance of ...
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    H.E.S.S. reveals a lack of TeV emission from the supernova remnant Puppis A 

    Abramowski, A.; Böttcher, M.; Davids, I.D.; Ivascenko, A.; Krüger, P.P.; Pekeur, N.W.; Spanier, F.; Sushch, I.; Venter, C.; Vorster, M. (EDP Sciences, 2015)
    Context: Puppis A is an interesting ~4 kyr-old supernova remnant (SNR) that shows strong evidence of interaction between the forward shock and a molecular cloud. It has been studied in detail from radio frequencies to ...
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    Probing the gamma-ray emission from HESS J1834-087 using H.E.S.S. and Fermi LAT observations 

    Abramowski, A.; Böttcher, M.; Casanova, S.; Davids, I.D.; Krüger, P.P.; Pekeur, N.W.; Sushch, I.; Venter, C.; Vorster, M. (EDP Sciences, 2015)
    Aims: Previous observations with the High Energy Stereoscopic System (H.E.S.S.) have revealed an extended very-high-energy (VHE; E> 100 GeV) γ-ray source, HESS J1834−087, coincident with the supernova remnant (SNR) W41. ...

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    AuthorBöttcher, M. (3)Davids, I.D. (3)
    Pekeur, N.W. (3)
    Sushch, I. (3)Abramowski, A. (2)Ivascenko, A. (2)Krüger, P.P. (2)Spanier, F. (2)Venter, C. (2)Vorster, M. (2)... View MoreSubject
    acceleration of particles (3)
    cosmic rays (2)radiation mechanisms: non-thermal (2)gamma rays: ISM (1)gamma rays: stars (1)ISM: clouds (1)ISM: individual objects: Puppis A (1)ISM: supernova remnants (1)stars: individual: 1FGL J1018.6-5856 (1)X-rays: binaries (1)... View MoreDate Issued2015 (3)

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