Abstract
We present 1.4-2.5 μm integral field spectroscopy of 16 stars in the Braid Nebula star formation region in Cygnus OB7. These data form one aspect of a large-scale multiwavelength survey aimed at determining an unbiased estimate of the number, mass distribution, and evolutionary state of the young stars within this 1 deg2 area of the previously poorly studied Lynds 1003 molecular cloud. Our new spectroscopic data, when combined with Two Micron All Sky Survey near-IR photometry, provide evidence of membership of many of these objects in the regions' pre-main-sequence population. We discuss both the characteristics of the young stars found in the region and the level of starforming activity present. © 2009. The American Astronomical Society. All rights reserved.
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Aspin, C., Beck, T. L., Pyo, T. S., Davis, C. J., Schieven, G. M., Khanzadyan, T., … Smith, M. D. (2009). Near-IR spectroscopy of young stars in the braid nebula star formation region in cygnus OB7. Astronomical Journal, 137(1), 431–449. https://doi.org/10.1088/0004-6256/137/1/431
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