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Discovery of X-Ray Counterparts to Gamma Ray Bursts by BeppoSAX

Published online by Cambridge University Press:  25 May 2016

L. Piro
L. Piro*
Affiliation:
Istituto Astrofisica Spaziale, C.N.R. Via Fosso del Cavaliere, 00131 Roma, Italy

Extract

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The nature of Gamma-Ray Burst (GRB) has been the object of many investigations but their origin has remained a mistery primarily for the difficulties in finding a counterpart. This difficulty derived from the intrinsically poor positioning capability of available GRB detectors.

Type
Session 3: Diagnostics of High Gravity Objects with X- and Gamma Rays
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 163 - 166
Copyright
Copyright © Kluwer 1998 

References

Boella, G. et al., A&A Supp. Ser., 122, 299–307 (1997)CrossRefGoogle Scholar
Boella, G., Chiappetti, L. et al., 1997b, A&AS, 122, 327 Google Scholar
Butler, R.C., et al. 1997, IAU Circular n. 6539.Google Scholar
Costa, E. et al. 1997, Nature, 387, 783 CrossRefGoogle Scholar
Jager, R., et al. 1997, A&A Suppl. Ser., 125, 557 CrossRefGoogle Scholar
Frontera, F., et al., A&A Supp. Ser., 122, 357–369 (1997) CrossRefGoogle Scholar
Frontera, et al. 1997b, IAUC 6637 Google Scholar
Parmar, A.N. et al. 1997, A&AS, 122, 309 Google Scholar
Piro, L., Scarsi, L. & Butler, R.C. 1995 SPIE 2517, 169 Google Scholar
Piro, L. et al. 1997, IAU Circ. 6617 Google Scholar
Piro, L. et al. 1997b, A&AL, in press (astro-ph/9710355) Google Scholar
Piro, et al. 1997c, A&A, in press (astro-ph/9707215) Google Scholar
Yoshida, A et al. 1997 IAUC 6593 Google Scholar