From the gamma-ray burst to its afterglow with BeppoSAX

Details From the gamma-ray burst to its afterglow with BeppoSAX From the gamma-ray burst to its afterglow with BeppoSAX

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...191.5501p&link_type=abstract

American Astronomical Society, 191st AAS Meeting, #55.01; Bulletin of the American Astronomical Society, Vol. 29, p.1303

Astronomy and Astrophysics

Astronomy

2

Scientific paper

The combination of the broad band narrow field instruments, the wide field cameras and gamma-ray burst monitor along with the operational capabilities of the whole BeppoSAX mission provides an unprecedented opportunity to study gamma-ray bursts. Along with the fast detection and precise positioning of these events, we will show how the gamma-ray burst evolves from time scales of seconds (i.e. the GRB proper) up to days (i.e. the afterglow) for the GRBs observed so far by all BeppoSAX instruments.

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