A Blind All-sky Search for Star Clusters in Gaia EDR3: 886 Clusters within 1.2 kpc of the Sun

Although previous searches for star clusters have been very successful, many clusters are likely still omitted, especially at high-Galactic-latitude regions. In this work, based on the astrometry of Gaia EDR3, we searched nearby ( ϖ > 0.8 mas) all-sky regions, obtaining 886 star clusters, of whic...

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Published inThe Astrophysical journal. Supplement series Vol. 262; no. 1; pp. 7 - 22
Main Authors He, Zhihong, Wang, Kun, Luo, Yangping, Li, Jing, Liu, Xiaochen, Jiang, Qingquan
Format Journal Article
LanguageEnglish
Published Saskatoon The American Astronomical Society 01.09.2022
IOP Publishing
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ISSN0067-0049
1538-4365
1538-4365
DOI10.3847/1538-4365/ac7c17

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Abstract Although previous searches for star clusters have been very successful, many clusters are likely still omitted, especially at high-Galactic-latitude regions. In this work, based on the astrometry of Gaia EDR3, we searched nearby ( ϖ > 0.8 mas) all-sky regions, obtaining 886 star clusters, of which 270 candidates have not been cataloged before. At the same time, we have presented the physical parameters of the clusters by fitting theoretical isochrones to their optical magnitudes. More halo members and expanding structures in many star clusters were also found. Most of the new objects are young clusters that are less than 100 million years old. Our work greatly increased the sample size and physical parameters of star clusters in the solar neighborhood, in particular, 46 clusters are newly found with ∣ b ∣ > 20°, which represents a nearly threefold increase in the number of clusters at high-Galactic-latitude regions.
AbstractList Although previous searches for star clusters have been very successful, many clusters are likely still omitted, especially at high-Galactic-latitude regions. In this work, based on the astrometry of Gaia EDR3, we searched nearby (ϖ > 0.8 mas) all-sky regions, obtaining 886 star clusters, of which 270 candidates have not been cataloged before. At the same time, we have presented the physical parameters of the clusters by fitting theoretical isochrones to their optical magnitudes. More halo members and expanding structures in many star clusters were also found. Most of the new objects are young clusters that are less than 100 million years old. Our work greatly increased the sample size and physical parameters of star clusters in the solar neighborhood, in particular, 46 clusters are newly found with ∣b∣ > 20°, which represents a nearly threefold increase in the number of clusters at high-Galactic-latitude regions.
Although previous searches for star clusters have been very successful, many clusters are likely still omitted, especially at high-Galactic-latitude regions. In this work, based on the astrometry of Gaia EDR3, we searched nearby ( ϖ > 0.8 mas) all-sky regions, obtaining 886 star clusters, of which 270 candidates have not been cataloged before. At the same time, we have presented the physical parameters of the clusters by fitting theoretical isochrones to their optical magnitudes. More halo members and expanding structures in many star clusters were also found. Most of the new objects are young clusters that are less than 100 million years old. Our work greatly increased the sample size and physical parameters of star clusters in the solar neighborhood, in particular, 46 clusters are newly found with ∣ b ∣ > 20°, which represents a nearly threefold increase in the number of clusters at high-Galactic-latitude regions.
Author Jiang, Qingquan
Luo, Yangping
Li, Jing
He, Zhihong
Liu, Xiaochen
Wang, Kun
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Snippet Although previous searches for star clusters have been very successful, many clusters are likely still omitted, especially at high-Galactic-latitude regions....
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SubjectTerms Astrometry
Latitude
Open star clusters
Parameters
Physical properties
Solar neighborhood
Star clusters
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Title A Blind All-sky Search for Star Clusters in Gaia EDR3: 886 Clusters within 1.2 kpc of the Sun
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