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Cited article:
V. V. Gvaramadze
A&A, 415 3 (2004) 1073-1078
Published online: 2004-02-13
This article has been cited by the following article(s):
14 articles
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Proper Motions of PSRs B1757−24 and B1951+32: Implications for Ages and Associations
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Discovery of Extended Emission around the Pulsar B0355+54
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The Pulsar Wind Nebula of the Geminga Pulsar
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Are radio pulsars the progenitors of anomalous X-ray pulsars and soft gamma repeaters?
F. K. Kasumov, A. O. Allakhverdiev and A. I. Asvarov Astronomy Letters 32 (5) 308 (2006) https://doi.org/10.1134/S1063773706050045
On the complex X-ray structure tracing the motion of Geminga
A. De Luca, P. A. Caraveo, F. Mattana, A. Pellizzoni and G. F. Bignami Astronomy & Astrophysics 445 (1) L9 (2006) https://doi.org/10.1051/0004-6361:200500217
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J. A. Blazek, B. M. Gaensler, S. Chatterjee, et al. The Astrophysical Journal 652 (2) 1523 (2006) https://doi.org/10.1086/507938
X‐Ray Spectroscopy of PSR B1951+32 and Its Pulsar Wind Nebula
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Bow shocks around pulsars and neutron stars
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Astrophysics in 2004
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Radio Pulsars as Progenitors of Anomalous X-Ray Pulsars and Soft Gamma-Ray Repeaters: Magnetic Field Evolution through Pulsar Glitches
J. R. Lin and S. N. Zhang The Astrophysical Journal 615 (2) L133 (2004) https://doi.org/10.1086/426316
The Mouse that Soared: High‐Resolution X‐Ray Imaging of the Pulsar‐powered Bow Shock G359.23−0.82
B. M. Gaensler, E. van der Swaluw, F. Camilo, et al. The Astrophysical Journal 616 (1) 383 (2004) https://doi.org/10.1086/424906