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Cited article:

Comptonization of Cosmic Microwave Background by Cold Ultrarelativistic Electron-Positron Pulsar Wind and Origin of ~130 GeV Lines

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Ukrainian Journal of Physics 61 (2) 178 (2016)
https://doi.org/10.15407/ujpe61.02.0178

A luminosity constraint on the origin of unidentified high energy sources

J M Siegal-Gaskins, V Pavlidou, A V Olinto, C Brown and B D Fields
Journal of Physics G: Nuclear and Particle Physics 36 (5) 055201 (2009)
https://doi.org/10.1088/0954-3899/36/5/055201

XMM‐NewtonObservations Reveal the X‐Ray Counterpart of the Very High Energy Gamma‐Ray Source HESS J1640−465

S. Funk, J. A. Hinton, G. Puhlhofer, et al.
The Astrophysical Journal 662 (1) 517 (2007)
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A microquasar model applied to unidentified gamma-ray sources

V. Bosch-Ramon, J. M. Paredes, G. E. Romero and D. F. Torres
Astronomy & Astrophysics 446 (3) 1081 (2006)
https://doi.org/10.1051/0004-6361:20052913

Discovery of Luminous Pulsed Hard X‐Ray Emission from Anomalous X‐Ray Pulsars 1RXS J1708−4009, 4U 0142+61, and 1E 2259+586 byINTEGRALandRXTE

L. Kuiper, W. Hermsen, P. R. den Hartog and W. Collmar
The Astrophysical Journal 645 (1) 556 (2006)
https://doi.org/10.1086/504317

Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500

V Bosch-Ramon, J M Paredes, G E Romero and D F Torres
Chinese Journal of Astronomy and Astrophysics 5 (S1) 284 (2005)
https://doi.org/10.1088/1009-9271/5/S1/284

Multiwavelength Approach to Unidentified Gamma-Ray Sources

Shu Zhang, Werner Collmar and Volker Schönfelder
Multiwavelength Approach to Unidentified Gamma-Ray Sources 283 (2005)
https://doi.org/10.1007/1-4020-3881-X_28