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Simultaneous observations of SiO and H_2O masers toward known stellar SiO and/or H_2O maser sources

机译:同时观察SIO和H_2O粉碎剂朝向已知的恒星SIO和/或H_2O MASERS来源

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We present the results of simultaneous observations of SiO v = 1, 2, ~(29)SiO v = 0, J = 1?0 and H_2O 6_(16)-5_(23) maser lines toward 318 known stellar SiO and/or H_2O maser sources using the Yonsei 21-m radio telescope of the Korean VLBI Network. Toward 166 known SiO and H_2O maser sources, both SiO and H_2O maser emissions were detected from 112 sources giving a detection rate of 67.5 %. On the other hand, toward 152 known H_2O-only maser sources, both SiO and H_2O maser emissions were detected from 62 sources, giving a detection rate of 40.8 %. Characteristics of all observed sources in the IRAS two-color diagram is investigated including their evolutionary sequence and mutual relations between SiO and H_2O maser properties.
机译:我们介绍了SiO v = 1,2,〜(29)SiO v = 0,J = 1〜0和H_2O 6_(16)-5_(23)朝向318已知恒星SIO和/或的MASER线的结果的结果H_2O MASERS使用韩国VLBI网络的Yonsi 21-M射频望远镜。朝向166名已知的SIO和H_2O蒙皮源,从112个源检测到SIO和H_2O蒙皮排放,均可检测率为67.5%。另一方面,朝向152个已知的H_2O的爆发源,从62个源检测到SIO和H_2O蒙皮排放,检测率为40.8%。研究了IRAS双色图中所有观察到的源的特征,包括它们在SiO和H_2O Maser性质之间的进化序列和相互关系。

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