本文根据NGC7538的红外和分子谱线观测结果,对红外源的热结构及成协气体的热平衡进行了计算和分析。得出尘埃温度随半径的分布T_d a r^(-0.36)其峰值温度略高于已有观测结果,并发现除中心源附近区域外,大部分区域内不再满足尘埃通过碰...本文根据NGC7538的红外和分子谱线观测结果,对红外源的热结构及成协气体的热平衡进行了计算和分析。得出尘埃温度随半径的分布T_d a r^(-0.36)其峰值温度略高于已有观测结果,并发现除中心源附近区域外,大部分区域内不再满足尘埃通过碰撞向气体输入能量的基本条件。本文计算了NGC7538气体的冷却串及多种机制的加热作用,结果表明宇宙线、坍缩及双极扩散等机制的加热率相对较小,而尘埃通过光电作用对气体的加热可能是气体的重要热源。展开更多
We present high angular resolution images of both NH3 (1, 1) and (2, 2) lines toward NGC 7538 IRS 1. The density and velocity-position plots have been used to study the interaction among the outflows, winds and their ...We present high angular resolution images of both NH3 (1, 1) and (2, 2) lines toward NGC 7538 IRS 1. The density and velocity-position plots have been used to study the interaction among the outflows, winds and their environment. For the first time we have found an expanding half-shell of molecular gas around the HII region associated with IRS 1, which may be produced by the interaction of the bipolar outflows and the winds originating in IRS 1-3, and optical HII region NGC 7538 with ambient molecular gas.展开更多
文摘本文根据NGC7538的红外和分子谱线观测结果,对红外源的热结构及成协气体的热平衡进行了计算和分析。得出尘埃温度随半径的分布T_d a r^(-0.36)其峰值温度略高于已有观测结果,并发现除中心源附近区域外,大部分区域内不再满足尘埃通过碰撞向气体输入能量的基本条件。本文计算了NGC7538气体的冷却串及多种机制的加热作用,结果表明宇宙线、坍缩及双极扩散等机制的加热率相对较小,而尘埃通过光电作用对气体的加热可能是气体的重要热源。
基金Supported by the National Natural Science Foundation of China.
文摘We present high angular resolution images of both NH3 (1, 1) and (2, 2) lines toward NGC 7538 IRS 1. The density and velocity-position plots have been used to study the interaction among the outflows, winds and their environment. For the first time we have found an expanding half-shell of molecular gas around the HII region associated with IRS 1, which may be produced by the interaction of the bipolar outflows and the winds originating in IRS 1-3, and optical HII region NGC 7538 with ambient molecular gas.
