Literature DB >> 15790849

A new population of very high energy gamma-ray sources in the Milky Way.

F Aharonian1, A G Akhperjanian, K-M Aye, A R Bazer-Bachi, M Beilicke, W Benbow, D Berge, P Berghaus, K Bernlöhr, C Boisson, O Bolz, C Borgmeier, I Braun, F Breitling, A M Brown, J Bussons Gordo, P M Chadwick, L-M Chounet, R Cornils, L Costamante, B Degrange, A Djannati-Ataï, L O'C Drury, G Dubus, T Ergin, P Espigat, F Feinstein, P Fleury, G Fontaine, S Funk, Y A Gallant, B Giebels, S Gillessen, P Goret, C Hadjichristidis, M Hauser, G Heinzelmann, G Henri, G Hermann, J A Hinton, W Hofmann, M Holleran, D Horns, O C de Jager, I Jung, B Khélifi, Nu Komin, A Konopelko, I J Latham, R Le Gallou, A Lemière, M Lemoine, N Leroy, T Lohse, A Marcowith, C Masterson, T J L McComb, M de Naurois, S J Nolan, A Noutsos, K J Orford, J L Osborne, M Ouchrif, M Panter, G Pelletier, S Pita, G Pühlhofer, M Punch, B C Raubenheimer, M Raue, J Raux, S M Rayner, I Redondo, A Reimer, O Reimer, J Ripken, L Rob, L Rolland, G Rowell, V Sahakian, L Saugé, S Schlenker, R Schlickeiser, C Schuster, U Schwanke, M Siewert, H Sol, R Steenkamp, C Stegmann, J-P Tavernet, R Terrier, C G Théoret, M Tluczykont, D J van der Walt, G Vasileiadis, C Venter, P Vincent, B Visser, H J Völk, S J Wagner.   

Abstract

Very high energy gamma-rays probe the long-standing mystery of the origin of cosmic rays. Produced in the interactions of accelerated particles in astrophysical objects, they can be used to image cosmic particle accelerators. A first sensitive survey of the inner part of the Milky Way with the High Energy Stereoscopic System (HESS) reveals a population of eight previously unknown firmly detected sources of very high energy gamma-rays. At least two have no known radio or x-ray counterpart and may be representative of a new class of "dark" nucleonic cosmic ray sources.

Entities:  

Year:  2005        PMID: 15790849     DOI: 10.1126/science.1108643

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  1 in total

1.  Proper motion, spectra, and timing of PSR J1813-1749 using Chandra and NICER.

Authors:  Wynn C G Ho; Sebastien Guillot; P M Saz Parkinson; B Limyansky; C-Y Ng; Michał Bejger; Cristóbal M Espinoza; B Haskell; Gaurava K Jaisawal; C Malacaria
Journal:  Mon Not R Astron Soc       Date:  2020-09-01       Impact factor: 5.287

  1 in total

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