TeV gamma-ray observations of the young synchrotron-dominated SNRs G1.9+0.3 and G330.2+1.0 with HESS

A Abramowski, F Aharonian,F Ait Benkhali,A G Akhperjanian, E Anguener,G Anton, S Balenderan,A Balzer,A Barnacka,Y Becherini,J Becker Tjus,K Bernloehr, E Birsin,E Bissaldi,J Biteau,Monika Boettcher,C Boisson,J Bolmont,P Bordas,J Brucker,F Brun,P Brun,T Bulik,S Carrigan,S Casanova,M Cerruti,P M Chadwick,R Chalmecalvet,R C G Chaves,A Cheesebrough,M Chretien,S Colafrancesco,G Cologna,J Conrad,C Couturier,Yi Cui,M Dalton,M K Daniel,I D Davids,B Degrange,C Deil,P Dewilt,H J Dickinson, A Djannatiatai,W Domainko,L O C Drury,G Dubus,K Dutson,J Dyks,M Dyrda,T Edwards,K Egberts,P Eger,P Espigat,C Farnier,S J Fegan,F Feinstein,M V Fernandes,David Iturbe Fernandez, A Fiasson,G Fontaine,A Foerster, M Fuessling, M Gajdus,Y A Gallant, T Garrigoux,G Giavitto,B Giebels, J F Glicenstein,M H Grondin,M Grudzinska,S Haeffner,J Hahn,J S Harris, G Heinzelmann,G Henri,G Hermann, O Hervet, A Hillert,J A Hinton,W Hofmann,P Hofverberg,Manfred J Holler,D Horns, A Jacholkowska,C Jahn,M Jamrozy,M Janiak, F Jankowsky,I Jung,M A Kastendieck,K Katarzynski, U F Katz,S Kaufmann,B Khelifi,M Kieffer,S Klepser,D Klochkov, W Kluzniak,T Kneiske, D Kolitzus,Nu Komin,K Kosack,S Krakau, F Krayzel,P P Krueger,H Laffon,G Lamanna, J Lefaucheur,A Lemiere, M Lemoinegoumard,J P Lenain,D Lennarz, T Lohse,A Lopatin, C C Lu,V Marandon,A Marcowith,Robert G Marx,G Maurin,N Maxted,M Mayer, T J L Mccomb,J Mehault,P J Meintjes, U Menzler,Michael Meyer,R Moderski,M K Mohamed,E Moulin, T Murach, C L Naumann,M De Naurois,J Niemiec,S J Nolan, L Oakes,S Ohm,E De Ona Wilhelmi,B Opitz,M Ostrowski,I Oya, M Panter,R D Parsons,M Paz Arribas,N W Pekeur,G Pelletier,Jorge Perez,P O Petrucci,B Peyaud,S Pita,H Poon,G Puehlhofer,M Punch,A Quirrenbach,Stephen S Raab,M Raue, A Reimer,O Reimer,M Renaud,R De Los Reyes,F Rieger,L Rob,C Romoli, S Rosierlees,G Rowell,B Rudak,C B Rulten,V Sahakian,D Sanchez,A Santangelo, R Schlickeiser,F Schuessler, A Schulz,U Schwanke,S Schwarzburg,S Schwemmer,H Sol,G Spengler,F Spies,L Stawarz,R Steenkamp,C Stegmann,F Stinzing,K Stycz,I Sushch,A Szostek,J P Tavernet,T Tavernier,A M Taylor,R Terrier, M Tluczykont, C Trichard,K Valerius,C Van Eldik,B Van Soelen,G Vasileiadis,C Venter,Ana Luiza Davila Viana,P Vincent,H J Voelk,F Volpe,M Vorster, T Vuillaume,Stefan Wagner,P Wagner,M J Ward,M Weidinger,Q Weitzel,R J White,A Wierzcholska,P Willmann, A Woernlein,D J Wouters,V Zabalza,M Zacharias,A Zajczyk,A A Zdziarski,A Zech,H S Zechlin

Monthly Notices of the Royal Astronomical Society（2014）

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摘要

The non-thermal nature of the X-ray emission from the shell-type supernova remnants (SNRs) G1.9+0.3 and G330.2+1.0 is an indication of intense particle acceleration in the shock fronts of both objects. This suggests that the SNRs are prime candidates for very-high-energy (VHE; E > 0.1 TeV) γ-ray observations. G1.9+0.3, recently established as the youngest known SNR in the Galaxy, also offers a uni...

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关键词

radiation mechanisms: non-thermal,ISM: individual objects: SNR G1.9+0.3,ISM: individual objects: SNR G330.2+1.0,ISM: magnetic fields,ISM: supernova remnants,gamma-rays: ISM

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