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°. 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...
Aims. According to some estimations, there are as many as 100 000 open clusters in the Galaxy, but l...
Despite having data for over 10 ^9 stars from Gaia, less than 10 ^4 star clusters and candidates hav...
Open clusters are convenient probes of the structure and history of the Galactic disk. They are also...
The astrometric satellite Gaia recently released part of its third data set, which provides a good o...
Context. Data from the Gaia satellite are revolutionising our understanding of the Milky Way. With e...
Gaia data is providing a unique opportunity to explore the structure of the Milky Way by discovering...
International audienceContext. Open clusters are key targets for studies of Galaxy structure and evo...
Context. The Gaia Data Release 2 (DR2) provided an unprecedented volume of precise astrometric and e...
[Context] The improvements in the precision of the published data in Gaia EDR3 with respect to Gaia ...
Aims. According to some estimations, there are as many as 100 000 open clusters in the Galaxy, but l...
We report 541 new open cluster candidates in Gaia EDR3 through revisiting the cluster results from a...
Context. Open clusters are key targets for studies of Galaxy structure and evolution, and stellar ph...
Gaia is revolutionising our understanding of open clusters in the Milky Way. Since the release of DR...
International audienceContext. The publication of the Gaia Data Release 2 (Gaia DR2) opens a new era...
International audienceContext. Open clusters (OCs) are popular tracers of the structure and evolutio...
Aims. According to some estimations, there are as many as 100 000 open clusters in the Galaxy, but l...
Despite having data for over 10 ^9 stars from Gaia, less than 10 ^4 star clusters and candidates hav...
Open clusters are convenient probes of the structure and history of the Galactic disk. They are also...
The astrometric satellite Gaia recently released part of its third data set, which provides a good o...
Context. Data from the Gaia satellite are revolutionising our understanding of the Milky Way. With e...
Gaia data is providing a unique opportunity to explore the structure of the Milky Way by discovering...
International audienceContext. Open clusters are key targets for studies of Galaxy structure and evo...
Context. The Gaia Data Release 2 (DR2) provided an unprecedented volume of precise astrometric and e...
[Context] The improvements in the precision of the published data in Gaia EDR3 with respect to Gaia ...
Aims. According to some estimations, there are as many as 100 000 open clusters in the Galaxy, but l...
We report 541 new open cluster candidates in Gaia EDR3 through revisiting the cluster results from a...
Context. Open clusters are key targets for studies of Galaxy structure and evolution, and stellar ph...
Gaia is revolutionising our understanding of open clusters in the Milky Way. Since the release of DR...
International audienceContext. The publication of the Gaia Data Release 2 (Gaia DR2) opens a new era...
International audienceContext. Open clusters (OCs) are popular tracers of the structure and evolutio...
Aims. According to some estimations, there are as many as 100 000 open clusters in the Galaxy, but l...
Despite having data for over 10 ^9 stars from Gaia, less than 10 ^4 star clusters and candidates hav...
Open clusters are convenient probes of the structure and history of the Galactic disk. They are also...