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Probing the nature of dark GRBs with the exceptional burst GRB 060108(*)

dc.contributor.authorZane, S.
dc.contributor.authorMonfardini, A.
dc.contributor.authorGuidorzi, C.
dc.contributor.authorMelandri, A.
dc.contributor.authorMalesani, D.
dc.contributor.authorOates, S. R.
dc.contributor.authorMundell, C. G.
dc.contributor.authorPiranomonte, S.
dc.contributor.authorPage, K. L.
dc.contributor.authorDE PASQUALE, Massımılıano
dc.date.accessioned2022-02-18T10:33:32Z
dc.date.available2022-02-18T10:33:32Z
dc.date.issued2006
dc.identifier.citationOates S. R. , Mundell C. G. , Piranomonte S., Page K. L. , DE PASQUALE M., Monfardini A., Melandri A., Zane S., Guidorzi C., Malesani D., "Probing the nature of dark GRBs with the exceptional burst GRB 060108(*)", NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-BASIC TOPICS IN PHYSICS, cilt.121, sa.12, ss.1547-1548, 2006
dc.identifier.issn2037-4895
dc.identifier.othervv_1032021
dc.identifier.otherav_a72c4d08-3b5b-49c8-aab0-287432004cd9
dc.identifier.urihttp://hdl.handle.net/20.500.12627/179468
dc.identifier.urihttps://doi.org/10.1393/ncb/i2007-10339-1
dc.description.abstractWe present observations of the optically dark burst GRB 060108, the 100th Swift burst. We find that the most likely explanation for the observed darkness is a combination of intrinsic faintness, a hard optical to X-ray spectrum and dust extinction.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectTemel Bilimler
dc.subjectDisiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.subjectFİZİK, MULTİDİSİPLİNER
dc.subjectFizik
dc.titleProbing the nature of dark GRBs with the exceptional burst GRB 060108(*)
dc.typeMakale
dc.relation.journalNUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-BASIC TOPICS IN PHYSICS
dc.contributor.department, ,
dc.identifier.volume121
dc.identifier.issue12
dc.identifier.startpage1547
dc.identifier.endpage1548
dc.contributor.firstauthorID3374337


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