Bocchino, F. (2005) Detection of thermal X-ray emission in the halo of the plerionic supernova remnant G21.5-0.9. Advances in Space Research, 35. 1003-1006 doi:10.1016/j.asr.2005.01.045

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Reference Type	Journal (article/letter/editorial)
Title	Detection of thermal X-ray emission in the halo of the plerionic supernova remnant G21.5-0.9
Journal	Advances in Space Research
Authors	Bocchino, F.		Author
Year	2005 (January)	Volume	35
Publisher	Elsevier BV
DOI	doi:10.1016/j.asr.2005.01.045Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	12567852	Long-form Identifier	mindat:1:5:12567852:2
GUID	0
Full Reference	Bocchino, F. (2005) Detection of thermal X-ray emission in the halo of the plerionic supernova remnant G21.5-0.9. Advances in Space Research, 35. 1003-1006 doi:10.1016/j.asr.2005.01.045
Plain Text	Bocchino, F. (2005) Detection of thermal X-ray emission in the halo of the plerionic supernova remnant G21.5-0.9. Advances in Space Research, 35. 1003-1006 doi:10.1016/j.asr.2005.01.045
In	(n.d.) Advances in Space Research Vol. 35. Elsevier BV

	*Matheson, Heather, Safi-Harb, Samar (2005) The plerionic supernova remnant G21.5-0.9: In and out. Advances in Space Research, 35. 1099-1105 doi:10.1016/j.asr.2005.04.050*
	*Bandiera, R., Bocchino, F. (2004) The X-ray halo of G21.5−0.9. Advances in Space Research, 33. 398-402 doi:10.1016/j.asr.2003.04.025*
	Raycheva, Nergis C., Sezer, Aytap (2022) A search for thermal X-ray emission from the composite supernova remnant G21.5–0.9 with Suzaku. Advances in Space Research, 69 (1) 531-537 doi:10.1016/j.asr.2021.11.016
	Miceli, M., Decourchelle, A., Ballet, J., Bocchino, F., Hughes, J., Hwang, U., Petre, R. (2008) A physical interpretation of the jet-like X-ray emission from supernova remnant W49B. Advances in Space Research, 41. 390-395 doi:10.1016/j.asr.2007.01.030
	Lu, Fang-Wu, Gao, Quan-Gui, Zhang, Li (2020) Two-zone Spatially Dependent Model of the Nonthermal Emission from Plerionic Supernova Remnant G21.5-0.9. The Astrophysical Journal, 889 (1). 30pp. doi:10.3847/1538-4357/ab5fda
	Matheson, Heather, Safi-Harb, Samar (2010) THE PLERIONIC SUPERNOVA REMNANT G21.5–0.9 POWERED BY PSR J1833–1034: NEW SPECTROSCOPIC AND IMAGING RESULTS REVEALED WITH THECHANDRA X-RAY OBSERVATORY. The Astrophysical Journal, 724 (1). 572-587 doi:10.1088/0004-637x/724/1/572
	Bocchino, F., van der Swaluw, E., Chevalier, R., Bandiera, R. (2005) The nature of the X-ray halo of the plerion G21.5–0.9 unveiled by XMM-Newton and Chandra. Astronomy & Astrophysics, 442 (2). 539-548 doi:10.1051/0004-6361:20052870
	Lai, Paul C. W., Ng, C.-Y., Bucciantini, Niccolo’ (2022) Magnetic Field Structure and Faraday Rotation of the Plerionic Supernova Remnant G21.5–0.9. The Astrophysical Journal, 930 (1) 1 doi:10.3847/1538-4357/ac63b1
	Park, Sangwook, Zhekov, Svetozar A., Burrows, David N., Garmire, Gordon P., McCray, Dick (2005) Supernova remnant 1987A: The latest report from the Chandra X-ray Observatory. Advances in Space Research, 35. 991-995 doi:10.1016/j.asr.2005.01.075
	*Xiao, Xiao, Chen, Yang (2008) A preliminary Chandra X-ray spectroscopy of the supernova remnant N132D. Advances in Space Research, 41. 416-423 doi:10.1016/j.asr.2007.03.071*
	Badenes, Carles, Bravo, Eduardo, Borkowski, Kazimierz J. (2005) A model grid for the spectral analysis of X-ray emission in young Type Ia supernova remnants. Advances in Space Research, 35. 987-990 doi:10.1016/j.asr.2005.01.019

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Bocchino, F. (2005) Detection of thermal X-ray emission in the halo of the plerionic supernova remnant G21.5-0.9. Advances in Space Research, 35. 1003-1006 doi:10.1016/j.asr.2005.01.045

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