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Cited article:

PSR B0656+14: the unified outlook from the infrared to X-rays

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Spectral characterization of the non-thermal X-ray emission of gamma-ray pulsars

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Monthly Notices of the Royal Astronomical Society 492 (1) 1025 (2020)

The relative and absolute timing accuracy of the EPIC-pn camera onXMM-Newton, from X-ray pulsations of the Crab and other pulsars

A. Martin-Carrillo, M. G. F. Kirsch, I. Caballero, et al.
Astronomy & Astrophysics 545 A126 (2012)


R. P. Mignani, G. G. Pavlov and O. Kargaltsev
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The X‐Ray Structure of the Pulsar Bow Shock G189.22+2.90 in the Supernova Remnant IC 443

B. M. Gaensler, S. Chatterjee, P. O. Slane, et al.
The Astrophysical Journal 648 (2) 1037 (2006)

Search for TeV emission from the region around PSR B1706–44 with the HESS experiment

F. Aharonian, A. G. Akhperjanian, K.-M. Aye, et al.
Astronomy & Astrophysics 432 (1) L9 (2005)

XMM‐NewtonObservations of PSR B1706−44

K. E. McGowan, S. Zane, M. Cropper, et al.
The Astrophysical Journal 600 (1) 343 (2004)

The Distance and Radius of the Neutron Star PSR B0656+14

Walter F. Brisken, S. E. Thorsett, A. Golden and W. M. Goss
The Astrophysical Journal 593 (2) L89 (2003)

Thermal Structure and Cooling of Superfluid Neutron Stars with Accreted Magnetized Envelopes

Alexander Y. Potekhin, Dmitry G. Yakovlev, Gilles Chabrier and Oleg Y. Gnedin
The Astrophysical Journal 594 (1) 404 (2003)