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. (arXiv:1904.01641v1 [astro-ph.GA])
<a href="http://arxiv.org/find/astro-ph/1/au:+Sitnik_T/0/1/0/all/0/1">T.G. Sitnik</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Egorov_O/0/1/0/all/0/1">O.V. Egorov</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lozinskaya_T/0/1/0/all/0/1">T.A. Lozinskaya</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Moiseev_A/0/1/0/all/0/1">A.V. Moiseev</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tatarnikov_A/0/1/0/all/0/1">A.M. Tatarnikov</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Vozyakova_O/0/1/0/all/0/1">O.V. Vozyakova</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wiebe_D/0/1/0/all/0/1">D.S. Wiebe</a>
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 [SII] 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.
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 [SII] 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.
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