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Cited article:

Timing analysis of the core of the Crab-like SNR G21.5–0.9

N. La Palombara, S. Mereghetti

A&A, 383 3 (2002) 916-918

Published online: 2002-03-15

DOI: https://doi.org/10.1051/0004-6361:20011839

This article has been cited by the following article(s):

Cross-calibration of the X-ray instruments onboard theChandra, INTEGRAL, RXTE,Suzaku, Swift, and XMM-Newtonobservatories using G21.5–0.9

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Astronomy & Astrophysics 525 A25 (2011)
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THE PLERIONIC SUPERNOVA REMNANT G21.5–0.9 POWERED BY PSR J1833–1034: NEW SPECTROSCOPIC AND IMAGING RESULTS REVEALED WITH THECHANDRA X-RAY OBSERVATORY

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The Astrophysical Journal 724 (1) 572 (2010)
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Hard X-ray observations of PSR J1833−1034 and its associated pulsar wind nebula

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Monthly Notices of the Royal Astronomical Society 393 (2) 527 (2009)
https://doi.org/10.1111/j.1365-2966.2008.14160.x

PSR J1833−1034: Discovery of the Central Young Pulsar in the Supernova Remnant G21.5–0.9

F. Camilo, S. M. Ransom, B. M. Gaensler, et al.
The Astrophysical Journal 637 (1) 456 (2006)
https://doi.org/10.1086/498386

Historical Evidence for the Birth of the Newly Discovered Pulsar PSR J1833–1034

Zhen-Ru Wang, Min Li and Yi Zhao
Chinese Journal of Astronomy and Astrophysics 6 (5) 625 (2006)
https://doi.org/10.1088/1009-9271/6/5/15

The nature of the X-ray halo of the plerion G21.5–0.9 unveiled by XMM-Newton and Chandra

F. Bocchino, E. van der Swaluw, R. Chevalier and R. Bandiera
Astronomy & Astrophysics 442 (2) 539 (2005)
https://doi.org/10.1051/0004-6361:20052870

Detection of thermal X-ray emission in the halo of the plerionic supernova remnant G21.5-0.9

F. Bocchino
Advances in Space Research 35 (6) 1003 (2005)
https://doi.org/10.1016/j.asr.2005.01.045