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X-ray and optical plateaus following the main bursts in GRBs and SNe Ⅱ-P: a hint about similar late injection behaviors?

X-ray and optical plateaus following the main bursts in GRBs and SNe Ⅱ-P: a hint about similar late injection behaviors?
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摘要 We analyze the emission plateaus in the X-ray afterglow light curves of gamma-ray bursts (GRBs) and those in the optical light curves of type Ⅱ plateau su- pernovae (SNe Ⅱ-P) in order to study whether they have similar late energy injection behaviors. We show that correlations of bolometric energies (or luminosities) between the prompt explosions and the plateaus for the two phenomena are similar. The energy emitted by SNe II-P are at the lower end of the range of possible energies for GRBs. The bolometric energies (or luminosities) in the prompt phase Eexpl (or Lexpl) and in the plateau phase E_plateau (or L_plateau) share relations of E_expl ∝E _0.73±0.14_plateau and L_expl ∝ L^-0.70_plateau. These results may indicate a similar late energy injection behavior that produces the observed plateaus in these two phenomena. We analyze the emission plateaus in the X-ray afterglow light curves of gamma-ray bursts (GRBs) and those in the optical light curves of type Ⅱ plateau su- pernovae (SNe Ⅱ-P) in order to study whether they have similar late energy injection behaviors. We show that correlations of bolometric energies (or luminosities) between the prompt explosions and the plateaus for the two phenomena are similar. The energy emitted by SNe II-P are at the lower end of the range of possible energies for GRBs. The bolometric energies (or luminosities) in the prompt phase Eexpl (or Lexpl) and in the plateau phase E_plateau (or L_plateau) share relations of E_expl ∝E _0.73±0.14_plateau and L_expl ∝ L^-0.70_plateau. These results may indicate a similar late energy injection behavior that produces the observed plateaus in these two phenomena.
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2013年第6期671-679,共9页 天文和天体物理学研究(英文版)
基金 supported by the National Basic Research Program of China (973 program, Grant Nos. 2012CB821800 and 2009CB824800) the National Natural Science Foundation of China(Grant Nos. 11225314, 11103026 and 10935001)
关键词 gamma rays: bursts -- supernovae: general -- methods: statistical gamma rays: bursts -- supernovae: general -- methods: statistical
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  • 1Arnett, W. D. 1980, ApJ, 237, 541.
  • 2Band, D., Matteson, J., Ford, L., et al. 1993, ApJ, 413, 281.
  • 3Barbon, R., Ciatti, F., & Rosino, L. 1979, A&A, 72, 287.
  • 4Bersten, M. C., & Hamuy, M. 2009, ApJ, 701,200.
  • 5Bersten, M. C., Benvenuto, O., & Hamuy, M. 2011, ApJ, 729, 61.
  • 6Bloom, J. S., Frail, D. A., & Sad, R. 2001, AJ, 121, 2879.
  • 7Burrows, A., Livne, E., Dessart, L., Ott, C. D., & Murphy, J. 2006, New Astron. Rev., 50, 487.
  • 8Chen, A., Yu, T., & Xu, R. 2007, ApJ, 668, L55.
  • 9Cui, X.-H., Liang, E.-W., Lv, H.-J., Zhang, B.-B., & Xu, R.-X. 2010, MNRAS, 401, 1465.
  • 10Dai, Z. G., & Lu, T. 1998a, Physical Review Letters, 81, 4301.

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