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  Detection of TeV emission from the intriguing composite SNR G327.1-1.1

Acero, F., Djannati-Atai, A., Foerster, A., Gallant, Y. A., Renaud, M., & H.E.S.S. collaboration (2011). Detection of TeV emission from the intriguing composite SNR G327.1-1.1. In Proceedings of the 32nd International Cosmic Ray Conference (pp. 184-186). Retrieved from http://www.ihep.ac.cn/englishttp://www.ihep.ac.cn/english/conference/icrc2011/paper/proc/v7.pdf.

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 Urheber:
Acero, F., Autor
Djannati-Atai, A.1, Autor           
Foerster, Andreas1, Autor           
Gallant, Y. A.1, Autor           
Renaud, M.1, Autor           
H.E.S.S. collaboration, Autor              
Affiliations:
1Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              

Inhalt

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Schlagwörter: High Energy Gamma rays ; H.E.S.S. ; Pulsar Wind Nebula ; SNR G327.1−1.1
 Zusammenfassung: The shock wave of supernova remnants (SNRs) and the wind termination shock in pulsar wind nebula (PWNe) are considered as prime candidates to accelerate the bulk of Galactic cosmic ray (CR) ions and electrons. The SNRs hosting a PWN (known as composite SNRs) provide excellent laboratories to test these hypotheses. The SNR G327.1– 1.1 belongs to this category and exhibits a shell and a bright central PWN, both seen in radio and X-rays. Interestingly, the radio observations of the PWN show an extended blob of emission and a curious narrow finger structure pointing towards the offset compact X-ray source indicating a possible fast moving pulsar in the SNR and/or an asymmetric passage of the reverse shock. We report here on the observations, for a total of 45 hours, of the SNR G327.1–1.1 with the H.E.S.S. telescope array which resulted in the detection of TeV -ray emission in spatial coincidence with the PWN.

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Sprache(n): eng - English
 Datum: 2011
 Publikationsstatus: Online veröffentlicht
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
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 Art des Abschluß: -

Veranstaltung

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Titel: ICRC2011: 32nd International Cosmic Ray Conference
Veranstaltungsort: Beijing, China
Start-/Enddatum: 2011-08-11 - 2011-08-20

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Titel: Proceedings of the 32nd International Cosmic Ray Conference
Genre der Quelle: Konferenzband
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Ort, Verlag, Ausgabe: -
Seiten: - Band / Heft: 7, OG2.2 Artikelnummer: - Start- / Endseite: 184 - 186 Identifikator: -