Panchromatic study of GRB 060124: From precursor to afterglow: From precursor to afterglow

P. Romano, S. Campana, G. Chincarini, J. Cummings, G. . Cusumano, S. T. Holland, V. Mangano, T. Mineo, K. L. Page, V. PaL'Shin, E. Rol, T. Sakamoto, B. Zhang, R. Aptekar, S. Barbier, S. Barthelmy, A. P. Beardmore, P. Boyd, D. N. Burrows, M. CapalbiE. E. Fenimore, P. Boyd, D. Frederiks, N. Gehrels, P. Giommi, M. R. Goad, O. Godet, S. Golenetskii, D. Guetta, J. A. Kennea, V. La Parola, D. Malesani, F. Marshall, A. Moretti, J. A. Nousek, P. T. O'Brien, J. P. Osborne, M. Perri, G. Tagliaferri

نتاج البحث: نشر في مجلةمقالةمراجعة النظراء

2 اقتباسات (Scopus)

ملخص

We present observations of GRB 060124, the first event for which both the prompt and the afterglow emission could be observed simultaneously and in their entirety by the three Swift instruments and by Konus-Wind. Thanks to these exceptional circumstances, the temporal and spectral properties of the prompt emission could be studied in the optical, X-ray and gamma-ray ranges (up to 2 MeV). While the X-ray emission (0.2-10 keV) clearly tracks the gamma-ray burst, the optical component follows a different pattern, likely indicating a different origin, possibly the onset of external shocks.

اللغة الأصليةالإنجليزيّة
الصفحات (من إلى)1067-1071
عدد الصفحات5
دوريةNUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS
مستوى الصوت121
رقم الإصدار10-11
المعرِّفات الرقمية للأشياء
حالة النشرنُشِر - 2006
منشور خارجيًانعم

بصمة

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