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

M. De Pasquale; S. Oates; A. Beardmore; K. Page; A. Blustin; S. Zane; M. Page; K. O'Mason; D. Burrows; D. Palmer; N. Gehrels; J. Nousek; P. Roming; P. Price; B. Zhang; S. Barthelmy; P. Boyd; R. Fink; S. Kobayashi; R. McNought; B. Peterson; J. Rich; S. Rosen; T. Sakamoto; B. Schmidt; J. Tueller; A. Wells; H. Ziaeepour; K. McGowan; X. T. Poole; A. Falcone; A. J. Blustin

doi:10.1393/ncb/i2007-10292-y

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

M. De Pasquale, S. Oates, A. Beardmore, K. Page, A. Blustin, S. Zane, M. Page, K. O'Mason, D. Burrows, D. Palmer, N. Gehrels, J. Nousek, P. Roming, P. Price, B. Zhang, S. Barthelmy, P. Boyd, R. Fink, S. Kobayashi, R. McNoughtB. Peterson, J. Rich, S. Rosen, T. Sakamoto, B. Schmidt, J. Tueller, A. Wells, H. Ziaeepour, K. McGowan, X. T. Poole, A. Falcone, A. J. Blustin

Research output: Contribution to journal › Article › peer-review

Abstract

Swift 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.

Original language	English (US)
Pages (from-to)	1471-1473
Number of pages	3
Journal	Nuovo Cimento della Societa Italiana di Fisica B
Volume	121
Issue number	12
DOIs	https://doi.org/10.1393/ncb/i2007-10292-y
State	Published - Dec 2006

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

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10.1393/ncb/i2007-10292-y

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De Pasquale, M., Oates, S., Beardmore, A., Page, K., Blustin, A., Zane, S., Page, M., O'Mason, K., Burrows, D., Palmer, D., Gehrels, N., Nousek, J., Roming, P., Price, P., Zhang, B., Barthelmy, S., Boyd, P., Fink, R., Kobayashi, S., ... Blustin, A. J. (2006). Energy injection in GRB afterglows: The case of Swift GRBs 050401, 050801 and 050802. Nuovo Cimento della Societa Italiana di Fisica B, 121(12), 1471-1473. https://doi.org/10.1393/ncb/i2007-10292-y

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abstract = "Swift 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.",

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year = "2006",

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doi = "10.1393/ncb/i2007-10292-y",

language = "English (US)",

volume = "121",

pages = "1471--1473",

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De Pasquale, M, Oates, S, Beardmore, A, Page, K, Blustin, A, Zane, S, Page, M, O'Mason, K, Burrows, D, Palmer, D, Gehrels, N, Nousek, J, Roming, P, Price, P, Zhang, B, Barthelmy, S, Boyd, P, Fink, R, Kobayashi, S, McNought, R, Peterson, B, Rich, J, Rosen, S, Sakamoto, T, Schmidt, B, Tueller, J, Wells, A, Ziaeepour, H, McGowan, K, Poole, XT, Falcone, A & Blustin, AJ 2006, 'Energy injection in GRB afterglows: The case of Swift GRBs 050401, 050801 and 050802', Nuovo Cimento della Societa Italiana di Fisica B, vol. 121, no. 12, pp. 1471-1473. https://doi.org/10.1393/ncb/i2007-10292-y

TY - JOUR

T1 - Energy injection in GRB afterglows

T2 - The case of Swift GRBs 050401, 050801 and 050802

AU - De Pasquale, M.

AU - Oates, S.

AU - Beardmore, A.

AU - Page, K.

AU - Blustin, A.

AU - Zane, S.

AU - Page, M.

AU - O'Mason, K.

AU - Burrows, D.

AU - Palmer, D.

AU - Gehrels, N.

AU - Nousek, J.

AU - Roming, P.

AU - Price, P.

AU - Zhang, B.

AU - Barthelmy, S.

AU - Boyd, P.

AU - Fink, R.

AU - Kobayashi, S.

AU - McNought, R.

AU - Peterson, B.

AU - Rich, J.

AU - Rosen, S.

AU - Sakamoto, T.

AU - Schmidt, B.

AU - Tueller, J.

AU - Wells, A.

AU - Ziaeepour, H.

AU - McGowan, K.

AU - Poole, X. T.

AU - Falcone, A.

AU - Blustin, A. J.

PY - 2006/12

Y1 - 2006/12

N2 - Swift 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.

AB - Swift 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.

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JF - Nuovo Cimento della Societa Italiana di Fisica B

IS - 12

ER -

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

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