A multiwavelength study of Swift GRB 060111B constraining the origin of its prompt optical emission

Stratta, G.; Pozanenko, A.; Atteia, J.; Klotz, A.; Basa, S.; Gendre, B.; Verrecchia, F.; Boer, M.; Cutini, S.; Henze, M.; Holland, S.; Ibrahimov, M.; Ienna, F.; Khamitov, I.; Klose, S.; Rumyantsev, V.; Biryukov, V.; Sharapov, D.; Vachier, F.; Arnouts, S.; Perley, D.

doi:10.1051/0004-6361/200911981

A multiwavelength study of Swift GRB 060111B constraining the origin of its prompt optical emission

Stratta G., Pozanenko A., Atteia J. -., Klotz A., Basa S., Gendre B., ...Daha Fazla

ASTRONOMY & ASTROPHYSICS, cilt.503, sa.3, ss.783-795, 2009 (SCI-Expanded, Scopus)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 503 Sayı: 3
Basım Tarihi: 2009
Doi Numarası: 10.1051/0004-6361/200911981
Dergi Adı: ASTRONOMY & ASTROPHYSICS
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
Sayfa Sayıları: ss.783-795
Anahtar Kelimeler: gamma rays: bursts, radiation mechanisms: non-thermal, methods: data analysis, GAMMA-RAY BURST, LIGHT CURVES, LORENTZ FACTOR, AFTERGLOW, GALAXIES, DUST, ULTRAVIOLET, FLASH, GRB-021211, GRB-990123
Açık Arşiv Koleksiyonu: AVESİS Açık Erişim Koleksiyonu
Akdeniz Üniversitesi Adresli: Evet

Özet

Context. The detection of bright optical emission measured with good temporal resolution during the prompt phase of GRB 060111B makes this GRB a rare event that is especially useful for constraining theories of the prompt emission.