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Probing the Properties of the Pulsar Wind in the Gamma-Ray Binary HESS J0632+057 with NuSTAR and VERITAS Observations

A. Archer,W. Benbow,R. Bird,A. Brill,R. Brose,M. Buchovecky,J. L. Christiansen,A. J. Chromey,W. Cui,A. Falcone,Q. Feng,J. P. Finley,L. Fortson,A. Furniss,A. Gent,G. H. Gillanders,C. Giuri,O. Gueta,D. Hanna,T. Hassan,O. Hervet,J. Holder,G. Hughes,T. B. Humensky,P. Kaaret,N. Kelley-Hoskins,M. Kertzman,D. Kieda,M. Krause,M. J. Lang,G. Maier,P. Moriarty,R. Mukherjee,D. Nieto,M. Nievas-Rosillo,S. O'Brien,R. A. Ong,A. N. Otte,N. Park,A. Petrashyk,K. Pfrang,M. Pohl,R. R. Prado,E. Pueschel,J. Quinn,K. Ragan,P. T. Reynolds,D. Ribeiro,G. T. Richards,E. Roache,I. Sadeh,M. Santander,S. Schlenstedt,G. H. Sembroski,I. Sushch,A. Weinstein,P. Wilcox,A. Wilhelm,D. A. Williams,T. J. Williamson,C. J. Hailey,S. Mandel,K. Mori

The Astrophysical Journal（2020）

Cited 10|Views26
Key words
Gamma-ray sources,High mass X-ray binary stars,Gamma-ray astronomy,Particle astrophysics,Pulsars
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