Star-forming regions at the periphery of the supershell surrounding the Cyg OB1 association - II. ISM kinematics and YSOs in the star cluster vdB 130 region

被引:6
作者
Sitnik, T. G. [1 ]
Egorov, O. V. [1 ,2 ]
Lozinskaya, T. A. [1 ]
Moiseev, A. V. [1 ,2 ]
Tatarnikov, A. M. [1 ]
Vozyakova, O. V. [1 ]
Wiebe, D. S. [3 ]
机构
[1] Lomonosov Moscow State Univ, Sternberg Astron Inst, Univ Sky Pr 13, Moscow 119234, Russia
[2] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia
[3] Russian Acad Sci, Inst Astron INASAN, Pyatnitskaya Str 48, Moscow 119017, Russia
基金
俄罗斯基础研究基金会;
关键词
ISM: bubbles; ISM: clouds; ISM: evolution; stars: protostars; ISM: kinematics and dynamics; open clusters and associations: individual: vdB 130; CCD OBSERVATIONS; TELESCOPE; REDUCTION; EMISSION; NEBULA; GALAXY; GAS; SKY;
D O I
10.1093/mnras/stz986
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an observational study of small-scale feedback processes operating in the star-forming region located in the wall of the expanding supershell around the Cyg OB1 association. The interstellar gas and dust content and pre-stellar populations in the vicinity of the open star cluster vdB 130 are analysed based on new optical and IR observations performed with the 6-m (3D spectroscopic mapping in the [S II] doublet) and 2.5-m (optical and NIR images) Russian telescopes along with the archival data of Spitzer and Herschel space telescopes. Analysing ionized gas kinematics and emission spectra, we discovered a compact region with supersonic motions. These motions may be caused either by stellar wind or a bipolar outflow from a protostellar disc. Young stellar objects were identified and classified in the area under study. Two star-forming regions were identified. One of them is a region of ongoing star formation in the head of the molecular cloud observed there and another one is a burst of star formation in the cloud tail.
引用
收藏
页码:2449 / 2461
页数:13
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