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GRB 041219A: Its host galaxy and its broad-band prompt optical-to-gamma-ray emission

  • Diego Götz
  • , Stefano Covino
  • , Romain Hascoët
  • , Alberto Fernández-Soto
  • , Frédéric Daigne
  • , Robert Mochkovitch
  • , Paolo Esposito

Résultats de recherche: Le chapitre dans un livre, un rapport, une anthologie ou une collectionContribution à une conférenceRevue par des pairs

Résumé

GRB 041219A is one of the longest and brightest gamma-ray bursts (GRBs) ever observed. It was discovered by the INTEGRAL satellite, and, thanks to a precursor happening about 300 s before the bulk of the burst, ground based telescopes were able to catch the rarely-observed prompt emission in the optical and in the near-infrared bands. Here we present the late-time multi-band near-infrared imaging data, collected at the CFHT, that allowed us to identify the host galaxy of the GRB as an under-luminous, irregular galaxy of ∼ 5 × 109M at best-fit redshift of z = 0.31 -0.26+0.54. In addition we model the broad-band prompt optical to γ-ray emission of GRB 041219A within the internal shock model, where we were able to reproduce the spectra and light curve invoking the synchrotron emission of relativistic electrons accelerated by a series of propagating shock waves inside a relativistic outflow.

langue originaleAnglais
titreGamma Ray Bursts 2010, GRB 2010
Pages261-264
Nombre de pages4
Les DOIs
étatPublié - 12 sept. 2011
Modification externeOui
EvénementGamma Ray Bursts 2010, GRB 2010 - Annapolis, MD, États-Unis
Durée: 1 nov. 20104 nov. 2010

Série de publications

NomAIP Conference Proceedings
Volume1358
ISSN (imprimé)0094-243X
ISSN (Electronique)1551-7616

Une conférence

Une conférenceGamma Ray Bursts 2010, GRB 2010
Pays/TerritoireÉtats-Unis
La villeAnnapolis, MD
période1/11/104/11/10

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