Young star clusters and the structure of the second Galactic quadrant II
DOI: 10.1093/mnras/stz1710
Bibcode: 2019MNRAS.488.2158M
Molina Lera, J. A.; Baume, G.; Gamen, R.
Argentina
Abstract
Galactic spiral arms are traced using young objects as giant molecular clouds, H II regions, OB stars, or young open/embedded clusters. To improve the knowledge of the Galactic structure in the second quadrant we selected, from more than 200 open clusters covered by the SDSS, a sample of 10 young stellar clusters to conduct a spectrophotometric study.
2019
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Monthly Notices of the Royal Astronomical Society
Gaia
7