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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?

作     者:Xiao-Hong Cui Ren-Xin Xu 

作者机构:National Astronomical Observatories Chinese Academy of Sciences School of Physics and State Key Laboratory of Nuclear Physics and Technology Peking University 

出 版 物:《Research in Astronomy and Astrophysics》 (天文和天体物理学研究(英文版))

年 卷 期:2013年第13卷第6期

页      面:671-679页

核心收录:

学科分类:07[理学] 070401[理学-天体物理] 0704[理学-天文学] 

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) 

主  题:gamma rays: bursts    supernovae: general    methods: statistical 

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.

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