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Energy injection in GRB afterglows: The case of Swift GRBs 050401, 050801 and 050802

dc.contributor.authorMcNought, R.
dc.contributor.authorZhang, B.
dc.contributor.authorBarthelmy, S.
dc.contributor.authorBoyd, P.
dc.contributor.authorFink, R.
dc.contributor.authorKobayashi, S.
dc.contributor.authorPeterson, B.
dc.contributor.authorRich, J.
dc.contributor.authorRosen, S.
dc.contributor.authorSakamoto, T.
dc.contributor.authorSchmidt, B.
dc.contributor.authorTueller, J.
dc.contributor.authorWells, A.
dc.contributor.authorZiaeepour, H.
dc.contributor.authorMcGowan, K.
dc.contributor.authorPoole, T.
dc.contributor.authorFalcone, A.
dc.contributor.authorBlustin, A. J.
dc.contributor.authorPalmer, D.
dc.contributor.authorO'Mason, K.
dc.contributor.authorBurrows, D.
dc.contributor.authorDE PASQUALE, Massımılıano
dc.contributor.authorOates, S.
dc.contributor.authorBeardmore, A.
dc.contributor.authorPage, K.
dc.contributor.authorBlustin, A.
dc.contributor.authorZane, S.
dc.contributor.authorPage, M.
dc.contributor.authorGehrels, N.
dc.contributor.authorNousek, J.
dc.contributor.authorRoming, P.
dc.contributor.authorPrice, P.
dc.date.accessioned2022-02-18T11:16:52Z
dc.date.available2022-02-18T11:16:52Z
dc.date.issued2006
dc.identifier.citationDE PASQUALE M., Oates S., Beardmore A., Page K., Blustin A., Zane S., Page M., O'Mason K., Burrows D., Palmer D., et al., "Energy injection in GRB afterglows: The case of Swift GRBs 050401, 050801 and 050802", NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-BASIC TOPICS IN PHYSICS, cilt.121, sa.12, ss.1471-1473, 2006
dc.identifier.issn2037-4895
dc.identifier.othervv_1032021
dc.identifier.otherav_e524c3b6-85ab-4d0f-9e24-c10adeee3121
dc.identifier.urihttp://hdl.handle.net/20.500.12627/180810
dc.identifier.urihttps://doi.org/10.1393/neb/i2007-10292-y
dc.description.abstractSwift unprecedented fast follow-up observations of gamma-ray bursts have allowed us to discover a new feature of GRB afterglows: a phase of shallow decay, usually attributed to energy injection in the burst ejecta, which can last for several thousands of seconds both in the X-ray and optical bands. Here I discuss this phase in the case of Swift GRBs 050401, 050801 and 050802.
dc.language.isoeng
dc.subjectDisiplinlerarası Fizik ve İlgili Bilim ve Teknoloji Alanları
dc.subjectFİZİK, MULTİDİSİPLİNER
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectTemel Bilimler
dc.titleEnergy injection in GRB afterglows: The case of Swift GRBs 050401, 050801 and 050802
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.startpage1471
dc.identifier.endpage1473
dc.contributor.firstauthorID3374311


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