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X-Ray Study of Crab-Like and Composite SNRs

Published online by Cambridge University Press:  25 May 2016

K. Torii ,
H. Tsunemi  and
P. Slane
K. Torii
Affiliation:
Osaka University
H. Tsunemi
Affiliation:
Osaka University
P. Slane
Affiliation:
Harvard-Smithsonian Center for Astrophysics

Extract

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We have presented X-ray observations of Crab-like supernova remnants (SNRs) (plerions) and (non-thermal) composite SNRs. We have observed several objects including 3C58, CTA1, and G292.0+1.8. Since space is limited, here we summarize results on G292.0+1.8. For the other objects, please refer to each publication (Slane et al. 1997; Torii et al. 1997).

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 258 - 259
Copyright
Copyright © Kluwer 1998 

References

Braun, R., Goss, W.M., Danziger, I.J. and Boksenberg, A. (1983) Supernova Remnants and Their X-ray Emissions. Reidel, Dordrecht.Google Scholar
Braun, R., Goss, W.M. and Roger, R.S. (1986) A&A , 162, 259 Google Scholar
Hughes, J.P. and Singh, K.P. (1994) ApJ , 422, 126 Google Scholar
Lyne, A.G. and Lorimer, D.R. (1994) Nature , 369, 127 Google Scholar
Saken, J.M., Fesen, R.A. and Shull, J.M. (1992) ApJS , 81, 715 Google Scholar
Sedov, L.I. (1993) Similarity and Dimensional Methods in Mechanics 10th Edition. CRC Press, Boca Raton.Google Scholar
Slane, P., Seward, F.D., Bandiera, R., Torii, K. and Tsunemi, H. (1997) ApJ , 485, 221 Google Scholar
Torii, K., Kinugasa, K., Hashimotodani, K., Tsunemi, H. and Slane, P.O. (1997) PASJ , submitted Google Scholar
Tuohy, I.R., Clark, D.H. and Burton, W.M. (1982) ApJL , 260, L65 Google Scholar