Nearby open clusters play a benchmark role in the observations related to the fundamental astrophysical processes, such as formation and evolution of stars and their planets. We used Gaia DR3 catalogue to place stars in the position-velocity space and re-evaluated memberships of young (<1Gyr) open clusters in the vicinity of the Sun (<500 pc). We re-examined their relative ages revealed from their colour-magnitude diagrams and rotation periods from the TESS data. This enables us to study the evolution of the luminosity function over time and speculate about the gradual evaporation and dispersal of their members into the Galactic disk. With the goal to make these results widely available to the professional and amateur communities, we are bu...
Based on the CCD observations of remote young open clusters NGC 2383, NGC 2384, NGC 4103, NGC 4755, ...
Context. Open clusters are very good tracers of the evolution of the Galactic disc. Thanks to Gaia, ...
Stellar clusters are gravitationally bound groups of stars. Astronomers distinguish two types of ste...
Context. Automated analyses of Gaia astrometric data have led to the discovery of many new high-qual...
Open clusters and associations are groups of young stars, respectively bound and unbound, that share...
The distribution of member stars in the surroundings of an Open Cluster (OC) can shed light on the p...
[Context] The distribution of member stars in the surroundings of an open cluster (OC) can shed ligh...
Open Clusters (OCs), and in particular the oldest ones, have been widely used to test formation and ...
[Context] Membership studies characterising open clusters (OCs) with Gaia data – most of them using ...
Context. In Gaia DR2, an unprecedented high level of precision has been reached at sub-milliarcsecon...
The goal of my work is to address the topic of the formation and evolution of the Galactic disk thro...
We provide a review of the current status of several topics on the ages, distances, and mass functio...
We report 541 new open cluster candidates in Gaia EDR3 through revisiting the cluster results from a...
We perform a systematic reanalysis of the age distribution of Galactic open star clusters. Using a c...
Open clusters are convenient probes of the structure and history of the Galactic disk. They are also...
Based on the CCD observations of remote young open clusters NGC 2383, NGC 2384, NGC 4103, NGC 4755, ...
Context. Open clusters are very good tracers of the evolution of the Galactic disc. Thanks to Gaia, ...
Stellar clusters are gravitationally bound groups of stars. Astronomers distinguish two types of ste...
Context. Automated analyses of Gaia astrometric data have led to the discovery of many new high-qual...
Open clusters and associations are groups of young stars, respectively bound and unbound, that share...
The distribution of member stars in the surroundings of an Open Cluster (OC) can shed light on the p...
[Context] The distribution of member stars in the surroundings of an open cluster (OC) can shed ligh...
Open Clusters (OCs), and in particular the oldest ones, have been widely used to test formation and ...
[Context] Membership studies characterising open clusters (OCs) with Gaia data – most of them using ...
Context. In Gaia DR2, an unprecedented high level of precision has been reached at sub-milliarcsecon...
The goal of my work is to address the topic of the formation and evolution of the Galactic disk thro...
We provide a review of the current status of several topics on the ages, distances, and mass functio...
We report 541 new open cluster candidates in Gaia EDR3 through revisiting the cluster results from a...
We perform a systematic reanalysis of the age distribution of Galactic open star clusters. Using a c...
Open clusters are convenient probes of the structure and history of the Galactic disk. They are also...
Based on the CCD observations of remote young open clusters NGC 2383, NGC 2384, NGC 4103, NGC 4755, ...
Context. Open clusters are very good tracers of the evolution of the Galactic disc. Thanks to Gaia, ...
Stellar clusters are gravitationally bound groups of stars. Astronomers distinguish two types of ste...