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Cited article:
D. C.-J. Bock , V. V. Gvaramadze
A&A, 394 2 (2002) 533-538
Published online: 2002-10-15
This article has been cited by the following article(s):
16 articles
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Detection of very-high-energyγ-ray emission from the vicinity of PSR B1706–44 and G 343.1–2.3 with H.E.S.S.
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A MULTIWAVELENGTH STUDY ON THE HIGH-ENERGY BEHAVIOR OF THEFERMI/LAT PULSARS
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Chen Wang, Dong Lai and J. L. Han The Astrophysical Journal 639 (2) 1007 (2006) https://doi.org/10.1086/499397
Supernova remnant S 147 and its associated neutron star(s)
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The Complex Wind Torus and Jets of PSR B1706−44
Roger W. Romani, C.‐Y. Ng, Richard Dodson and Walter Brisken The Astrophysical Journal 631 (1) 480 (2005) https://doi.org/10.1086/432527
Search for TeV emission from the region around PSR B1706–44 with the
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On the origin of the system PSR B 1757$\mathsf{-}$24/SNR G 5.4$\mathsf{-}$1.2
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Observational data on Galactic supernova remnants III: The supernova remnants within l = 270°-360°
O.H. Guseinov, A. Ankay and S.O. Tagieva Serbian Astronomical Journal (169) 65 (2004) https://doi.org/10.2298/SAJ0469065G
Fitting Pulsar Wind Tori
C.‐Y. Ng and Roger W. Romani The Astrophysical Journal 601 (1) 479 (2004) https://doi.org/10.1086/380486
An X‐Ray Search for Compact Central Sources in Supernova Remnants. I. SNR
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G093.3+6.9, G315.4−2.3, G084.2+0.8, and G127.1+0.5
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XMM‐NewtonObservations of PSR B1706−44
K. E. McGowan, S. Zane, M. Cropper, et al. The Astrophysical Journal 600 (1) 343 (2004) https://doi.org/10.1086/379787
The Association of PSR B1757–24 and the SNR G5.4–1.2
V. V. Gvaramadze Symposium - International Astronomical Union 218 77 (2004) https://doi.org/10.1017/S0074180900180635
Neutron Stars in Supernova Remnants and Beyond
Vasilii V. Gvaramadze Symposium - International Astronomical Union 214 141 (2003) https://doi.org/10.1017/S007418090019429X