Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-17T16:45:07.302Z Has data issue: false hasContentIssue false

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

Published online by Cambridge University Press:  25 May 2016

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

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Copyright
Copyright © Kluwer 1998 

References

Boella, G. et al., A&A Supp. Ser., 122, 299307 (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, 357369 (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