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Newly detected open clusters in the Galactic disk using Gaia EDR3
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abstract
The astrometric satellite Gaia recently released part of its third data set, which provides a good opportunity to hunt for more open clusters in the Milky Way. In this work, we conduct a blind search for open clusters in the Galactic disk using a sample-based clustering search method with high spatial resolution, which is especially suited to finding hidden targets. In addition to confirming 1930 previously known open clusters and 82 known globular clusters, 704 new stellar clusters are proposed as potential open clusters at Galactic latitudes of $|$b$|$ < 20 {deg}. For each of these new open clusters, we present the coordinates, detailed astrometric parameters, and ages, as well as the radial velocity, if available. Our blind search greatly increases the number of Galactic open clusters as objects of study and shows the incompleteness of the open cluster census across our Galaxy
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Mapping the reddening plane in the Galactic disk through interstellar extinction of open clusters
Open clusters trace a wavy reddening plane offset 15.7 pc below the Sun, whose absorbing layer has a mean thickness of about 201 pc and a cluster scale height of 87 pc.
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