天文学报
天文學報
천문학보
ACTA ASTRONOMICA SINICA
2001年
1期
16-21
,共6页
y射线暴%火球%演化%余辉
y射線暴%火毬%縯化%餘輝
y사선폭%화구%연화%여휘
GRB主暴后,火球继续膨胀,根据暴后火球的动力学演化方程,考虑电子的分布随时问的变化,通过数值求解,得到光学R波段和X射线余辉与时间t的关系.计算结果与观测结果相比较,符合得很好.最后,还讨论了火球+激波模型的不足.
GRB主暴後,火毬繼續膨脹,根據暴後火毬的動力學縯化方程,攷慮電子的分佈隨時問的變化,通過數值求解,得到光學R波段和X射線餘輝與時間t的關繫.計算結果與觀測結果相比較,符閤得很好.最後,還討論瞭火毬+激波模型的不足.
GRB주폭후,화구계속팽창,근거폭후화구적동역학연화방정,고필전자적분포수시문적변화,통과수치구해,득도광학R파단화X사선여휘여시간t적관계.계산결과여관측결과상비교,부합득흔호.최후,환토론료화구+격파모형적불족.
After the main part of a GRB, its fireball continuously expands. With the
hydrodynamic equations for the postburst fireball, the authors study the distribution of electrons, which changes with time. The equations are solved numerically and the relations of the flux density of Optical afterglow in R band as well as the X- ray afterglow with time have been obtained. The results fit the observations quite well. Finally the shortcomings of the fireball + blast model are discussed.