【摘要】 对ＩＲＡＳ ２３３８５＋６０５３进行了^１２ＣＯ Ｊ＝ １—０的成图观测，获得的谱线具有较宽的线翼，显示出其中高速气体的存在，证认其为外向流．对外向流参数及其驱动源的分析表明，它是一个与大质量年轻星体相关的高质量、高能量的外向流．利用ＣＯ谱线测量作为Ｔ_k的探测手段，对环境气体的热特性也进行了研究．Ｔ_Ｋ和Ｔ_Ｄ的比较表明，靠近这个红外源处不满足标准的Ｇｏｌｄｒｅｉｃｈ－Ｋｗａｎ能量图像，对其可能存在的加热机制进行了讨论．更多还原

【Abstract】 ¹²CO J = 1 - 0 mapping observations were made towards IRAS 23385+6053. The broad line wings observed revealed the presence of high-velocity gas activity in this source, which is identified as an outflow for the first time. The outflow parameters derived and the analysis of its driving source show it to be a massive, energetic outflow associated with a young stellar object （YSO） of very high mass. Using CO line measurements as a TK probe, the thermal properties of the ambient gas are also investigated.A comparison between Tk and TD shows that near this IRAS source the standard Goldreich-Kwan picture of energetic is not satisfied.Therefore alternative heating mechanisms are discussed.更多还原