Ammonia cores in high mass star formation regions

作者：Yuefang Wu, Qizhou Zhang, Wentao Yu, M. Miller, R. Q. Mao, K. Sun, Y. Wang · 发表于：Astronomy and Astrophysics · 年份：2006 · 被引用次数：58 · 研究领域：Astrophysics and Star Formation Studies、Molecular Spectroscopy and Structure、Atmospheric Ozone and Climate

We observed a sample of 35 water masers not coincident with known HII regions and/or low mass young stellar objects (YSOs) with the Effelsberg 100 m telescope in the = (1, 1), (2, 2), (3, 3) and (4, 4) transitions. Sixteen sources were detected in the NH3 emission. The detection rate is 46%. All these sixteen sources have NH3 (1, 1) and (2, 2) emission, among which four sources have NH3 (3, 3) emission. Comparing with the IRAS and the 2MASS data, we analyzed the relationship between the detection rate and the infrared color, the dust temperature and the source distance. All the detected sources were mapped and 17 cores were obtained (one source IRAS 20215+3725 has two cores). From the detected sources five cores do not coincide with radio continuum or IRAS and MSX point sources. Excluding one core that has no MSX data available, the remaining eleven cores are coincident with IRAS or MSX point sources. The typical size and mass of the cores are 1.6 pc and 1.5 103 , respectively. The average line widths of the NH3 (1, 1) and (2, 2) are 1.54 and 1.73 km s-1. The average kinetic temperature of the gas is about 19 K. These values are much larger than those of low mass cores. The NH3 cores that coincide with IRAS sources (referred to as Group I) have slightly larger line widths (1.65 and 1.75 km s-1 for the (1, 1) and (2, 2) lines, respectively) and larger masses ( ) than the mean values of the sample. For this type of core the kinetic temperature correlates with the line width. Th...