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Astronomy Reports, ISSN 1063-7729, 8/2019, Volume 63, Issue 8, pp. 642 - 651
Measurements of the flux densities of the supernova remnant G21.5-0.9 at 4840 and 8450 MHz were performed in 2013–2018 on the 32-m telescope of the Svetloe... 
Physics | Astronomy, Observations and Techniques | PULSAR | RADIO | SCALE | ASTRONOMY & ASTROPHYSICS | PSR J1833-1034 | DISCOVERY | Analysis | Spectra | Astronomy | Supernova | Supernova remnants | Fluctuations | Change detection | Moon | Variability | Flux | Power law
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2019, Volume 482, Issue 1, pp. 1031 - 1042
G21.5-0.9 is a plerionic supernova remnant (SNR) used as a calibration target for the Chandra X-ray telescope. The first observations found an extended halo... 
ISM: individual objects: G21.5-0.9 | X-rays: ISM | ISM: supernova remnants | ISM: individual objects: G21 | DISCOVERY | CRAB-NEBULA | PULSAR WIND | EVOLUTION | ASTRONOMY & ASTROPHYSICS | 5-0 | RADIO | ABSORPTION | EMISSION | HALO | PSR J1833-1034 | Physics - High Energy Astrophysical Phenomena
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 01/2011, Volume 525, Issue 17
Context. For many years, X-ray astronomy missions have used the Crab nebula as a celestial calibration source for the X-ray flux and spectral shape. However,... 
X-rays: individuals: G21.5-0.9 | instrumentation: detectors | IN-ORBIT PERFORMANCE | PHOTON IMAGING CAMERA | SUPERNOVA REMNANT G21.5-0.9 | SNR G21.5-0.9 | MISSION | PULSAR | DISCOVERY | BOARD SUZAKU | ASTRONOMY & ASTROPHYSICS | HALO | PSR J1833-1034
Journal Article
Current Science, ISSN 0011-3891, 09/2005, Volume 89, Issue 5, pp. 853 - 856
We report the discovery of a young pulsar associated with the supernova remnant G21.5-0.9, using the Giant Metrewave Radio Telescope (GMRT) located near Pune,... 
Giant Metrewave Radio Telescope | Pulsar | PSR J1833-1034 | Supernova remnant | CRAB-NEBULA | TELESCOPE | SEARCH | MULTIDISCIPLINARY SCIENCES | X-RAY OBSERVATIONS | supernova remnant | RADIO PULSARS | 3C-58 | pulsar
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/2014, Volume 789, Issue 1, pp. 1 - 12
Journal Article
Astrophysical Journal, ISSN 0004-637X, 11/2018, Volume 867, Issue 2, p. 141
We present a new pulsar wind nebula (PWN) model that solves both advection and diffusion of nonthermal particles in a self-consistent way to satisfy the... 
radiation mechanisms: non-thermal | ISM: individual objects (3C 58, G21.5-0.9) | stars: winds, outflows | magnetohydrodynamics (MHD) | pulsars: general | CALIBRATION | SUPERNOVA REMNANT G21.5-0.9 | COSMIC-RAY PROPAGATION | 3C-58 | CRAB-NEBULA | ACCELERATION | ORIGIN | EVOLUTION | ASTRONOMY & ASTROPHYSICS | PSR J1833-1034 | 3C 58
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2008, Volume 386, Issue 3, pp. 1411 - 1416
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2011, Volume 412, Issue 2, pp. 1221 - 1228
We report on sensitive new 1.4-GHz Very Large Array radio observations of the pulsar wind nebula G21.5−0.9, powered by PSR J1833−1034, and its environs. Our... 
ISM: supernova remnants | REMNANT G21.5-0.9 | SPECTRAL INDEX | WAVELENGTHS | ASTRONOMY & ASTROPHYSICS | CHANDRA | X-RAY HALO | INNER GALAXY | 3C-58 | PSR J1833-1034 | DISCOVERY | CRAB | Analysis | Astronomy | X-rays | Supernovae | Nebulae | Radio astronomy | Physics - Astrophysics of Galaxies
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 11/2011, Volume 741, Issue 1, pp. 40 - jQuery1323902167708='48'
Journal Article