HII区相关论文
利用高精度数值模拟的结果修正了高红移类星体(QSO)电离和加热中性气体的理论模拟,并预测了500 m口径球面射电望远镜(Five-hundred......
基于LAMOST(大天区面积多目标光纤光谱天文望远镜)DR3的单次曝光光谱,分析了集中在反银心方向H II区及H II候选区中的恒星和天光光......
射电连续谱偏振观测是探测银河系星际介质性质的有力工具.中德6 cm银道面偏振巡天使用新疆天文台南山站25 m射电望远镜对银道面银......
Arecibo银道面电离气体巡天(Survey of Ionized Gas in the Galaxy, made with theArecibo telescope-SIGGMA)对Arecibo望远镜全部......
在乌鲁木齐天文站的25m射电望远镜上，安装了一套新的谱线接收系统，其终端频谱分析器为声表面波频谱仪，在世界上这是第1次实际应用于射......
本文通过仙王座Sh2-140中年轻恒星成团形成及分布情况研究该区恒星形成的图景.在探究过程中,主要采用KPNO 4米多波段光学成像资料,......
The first mapping observations of the bipolar HII region S106 in HCN J = 3-2 line were made by KOSMA submillimeter teles......
提出用准直因子与分子外向流质量之间的关系，分子外向流动量变化率和质量变化率与中心源的光度关系，统计地推断作为外向流驱动源的中......
研究表明,在新形成大质量恒星辐射的影响下,分子云中会形成高密度的HⅡ区。近年来观测到一些非球对称彗星状致密HⅡ区,学者们为了......
We present the results of a high-resolution study with the Submillimeter Array(SMA)toward the massive star-forming compl......
本文作者用上海天文台的２５米天线和１２．２ＧＨｚ的接收系统，对银道面附近的一个ＨＩＩ区复合体Ｇ１８．２—０．３进行了射电连续谱观测．采用沿源运动轨迹，对观测曲线进行多......
本文利用IRAS资料,详细研究了HII区一分子云复合体S252中12μm频带的辐射强度随辐射场的变化.结果表明,为了解释过量的短波辐射,必......
Using the 13.7 m radio telescope at Delingha, the millimeter-wave radioobservatory of Purple Mountain Observatory, we ma......
We present a statistical analysis of 482 6.7 GHz methanol maser sourcesfrom the available literature, on their maser emi......
To investigate the physical properties of HII regions and some PNe about 4 in size, a DEFPOS Fabry-Perot spectrometer ha......
IRAS 22475+5939 has been well studied by previous astronomers, but we can still discover new characteristics about it, u......
We performed a multiwavelength study towards the infrared dark cloud(IRDC) G31.23+0.05 with new CO observations from Pur......
在 HII 区域沉浸的 Photoionized 喷气显示特殊性质，它使他们成为了 Herbig Haro (HH ) 流动的一个特殊范畴。如此的喷气系统的详细......
The 110-111 formaldehyde (H2CO) absorption line and H110α radio recombination line (H RRL) are observed towards the gia......
