6533b85afe1ef96bd12b8cc1

RESEARCH PRODUCT

The short GRB 051210 observed by Swift

V. La ParolaV. ManganoB. ZhangG. CusumanoT. MineoE. TrojaD. N. BurrowsS. CampanaM. CapalbiG. ChincariniP. GiommiA. MorettiM. PerriP. RomanoG. Tagliaferri

subject

Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstrophysics::Galaxy Astrophysics

description

We report on the short GRB051210 detected by the Swift-BAT. The light curve, on which we focus mainly, shows a hint of extended emission in the BAT energy range, a steep decay of the X-ray emission, without any flattening or break, and two small flares in the first 300 sec. The emission fades out after ~1000 s.

yearjournalcountryeditionlanguage
2007-01-29
10.1393/ncb/i2007-10299-4http://hdl.handle.net/10447/29892