We present the spectral and temporal analysis of the X-ray flash XRF 011030 observed with BeppoSAX. This event is characterized by a very long X-ray bursting activity that lasts about 1500 s, one of the longest ever observed by BeppoSAX. In particular, a precursor and a late flare are present in the light curve. We connect the late X-ray flare observed at about 1300 s to the afterglow emission observed by Chandra and associate it with the onset of the afterglow emission in the framework of external shock by a long duration engine activity. We find that the late X-ray flare and the broadband afterglow data, including optical and radio measurements, are consistent either with a fireball expanding in a wind environment or with a jetted fireball in an ISM.
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Max Planck Inst Solar Syst Res, Justus Von Liebig Weg 3, D-37077 Gottingen, GermanyMax Planck Inst Solar Syst Res, Justus Von Liebig Weg 3, D-37077 Gottingen, Germany
Chatzistergos, Theodosios
Krivova, Natalie A.
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Max Planck Inst Solar Syst Res, Justus Von Liebig Weg 3, D-37077 Gottingen, GermanyMax Planck Inst Solar Syst Res, Justus Von Liebig Weg 3, D-37077 Gottingen, Germany
Krivova, Natalie A.
Yeo, Kok Leng
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Max Planck Inst Solar Syst Res, Justus Von Liebig Weg 3, D-37077 Gottingen, GermanyMax Planck Inst Solar Syst Res, Justus Von Liebig Weg 3, D-37077 Gottingen, Germany
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Univ Jyvaskyla, Sch Business & Econ, FIN-40014 Jyvaskyla, Finland
Yrjo Jahnsson Fdn, FIN-00120 Helsinki, FinlandUniv Jyvaskyla, Sch Business & Econ, FIN-40014 Jyvaskyla, Finland
Hyytinen, Ari
Lahtonen, Jukka
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Univ Jyvaskyla, Sch Business & Econ, FIN-40014 Jyvaskyla, Finland
Res Inst Finnish Econ, FIN-00120 Helsinki, FinlandUniv Jyvaskyla, Sch Business & Econ, FIN-40014 Jyvaskyla, Finland
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Univ British Columbia, Vancouver, BC V5Z 1M9, Canada
Vancouver Coastal Hlth Authority, Vancouver, BC, CanadaUniv British Columbia, Vancouver, BC V5Z 1M9, Canada