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The puzzling temporally variable optical and X-ray afterglow of GRB 101024A

Identifieur interne : 006618 ( Main/Exploration ); précédent : 006617; suivant : 006619

The puzzling temporally variable optical and X-ray afterglow of GRB 101024A

Auteurs : B. Gendre [Italie] ; G. Stratta [Italie] ; M. Laas-Bourez [Australie] ; D. M. Coward [Australie] ; A. Klotz [France] ; S. Cutini [Italie] ; M. Boër [France] ; C. Stockdale [Australie]

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RBID : Pascal:11-0448002

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Abstract

Aims. We present the optical observations of the afterglow of the Swift burst GRB 101024A and try to reconcile these observations with the X-ray afterglow data of GRB 101024A using current afterglow models Methods. We employ early optical observations, using the Zadko Telescope combined with X-ray data, to compare them with the reverse shock/forward shock model. Results. The early optical light curve reveals a very unusual steep decay index of α ˜ 5. This is followed by a flattening and possibly a plateau phase coincident with a similar feature in the X-ray. We discuss these observations in the framework of the standard reverse shock/forward shock model and energy injection. The plateau phase might also be the signature of the formation of a new magnetar.


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Le document en format XML

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<div type="abstract" xml:lang="en">Aims. We present the optical observations of the afterglow of the Swift burst GRB 101024A and try to reconcile these observations with the X-ray afterglow data of GRB 101024A using current afterglow models Methods. We employ early optical observations, using the Zadko Telescope combined with X-ray data, to compare them with the reverse shock/forward shock model. Results. The early optical light curve reveals a very unusual steep decay index of α ˜ 5. This is followed by a flattening and possibly a plateau phase coincident with a similar feature in the X-ray. We discuss these observations in the framework of the standard reverse shock/forward shock model and energy injection. The plateau phase might also be the signature of the formation of a new magnetar.</div>
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