摘要
提出了一个改进的３Ｃ２７３中红外－毫米波爆发模型，计入在康普顿阶段和同步辐射阶段之间的过渡期间爆发源的加速，以便解释爆发上升段的细致演化，讨论了绝热阶段爆发的演化，并与１４．５ＧＨｚ观测作了比较．
An improved model for the IR-mm outbursts in 3C 273, taking into account the bulk acceleration of emitting sources during the transition between the Compton and synchrotron stages, is presented to explain the detailed evolution of the rising phase of outbursts. The evolution of the outbursts in the adiabatic stage is also derived and compared with the observations at 14.5 GHz.
基金
中国科学院天文委员会资助
