Pregled bibliografske jedinice broj: 984138
VARIABLE POLARIZATION MEASURED IN THE PROMPT EMISSION OF GRB 041219A USING IBIS ON BOARDINTEGRAL
VARIABLE POLARIZATION MEASURED IN THE PROMPT EMISSION OF GRB 041219A USING IBIS ON BOARDINTEGRAL // The Astrophysical Journal, 695 (2009), 2; L208-L212 doi:10.1088/0004-637x/695/2/l208 (međunarodna recenzija, članak, znanstveni)
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Naslov
VARIABLE POLARIZATION MEASURED IN THE PROMPT EMISSION OF GRB 041219A USING IBIS ON BOARDINTEGRAL
Autori
Götz, Diego ; Laurent, Philippe ; Lebrun, François ; Daigne, Frédéric ; Bošnjak, Željka
Izvornik
The Astrophysical Journal (0004-637X) 695
(2009), 2;
L208-L212
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
gamma rays: bursts, gamma rays: observations, polarization
Sažetak
Polarization measurements provide a direct insight into the nature of astrophysical processes. Unfortunately, only a few instruments are available for this kind of measurement at γ-ray energies, and the sources need to be very bright. Gamma-ray bursts (GRBs) are ideal candidates due to their large flux over limited time intervals, maximizing the available signal-to-noise ratio. To date a few polarization measurements have been reported, claiming a high degree of polarization in the prompt emission of GRBs but with low statistical evidence. We used the IBIS telescope on board the INTEGRAL satellite to measure the polarization of the prompt γ-ray emission of the long and bright GRB 041219A in the 200-800 keV energy band. We find a variable degree of polarization ranging from less than 4% over the first peak to 43% ± 25% for the whole second peak. Time resolved analysis of both peaks indicates a high degree of polarization, and the null average polarization in the first peak can be explained by the rapid variations observed in the polarization angle and degree. Our results are consistent with different models for the prompt emission of GRBs at these energies, but they favor synchrotron radiation from a relativistic outflow with a magnetic field, which is coherent on an angular size comparable with the angular size of the emitting region (~1/Γ). Indeed, this model has the best capabilities to maintain a high polarization level, and to produce the observed variability.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus