Hunting for Neighboring Open Clusters with Gaia DR3: 101 New Open Clusters within 500 pc
arXiv:2212.11034 · doi:10.3847/1538-4365/acadd6
Abstract
We systematically searched for open clusters in the solar neighborhood within 500 pc using pyUPMASK and HDBSCAN clustering algorithms based on {\it Gaia} DR3. Taking into consideration that the physical size for most open clusters is less than 50 pc, we adopted a slicing approach for different distance shells and identified 324 neighboring open clusters, including 223 reported open clusters and 101 newly discovered open clusters (named as OCSN, Open Cluster of Solar Neighborhood). Our discovery has increased the number of open clusters in the solar neighborhood by about 45\%. In this work, larger spatial extents and more member stars were attained for our cluster sample. We provided the member stars and the membership probabilities through the pyUPMASK algorithm for each cluster and derived their astrophysical, age, and structural parameters.
32 pages, 10 figures
References in corpus (23)
- astroquery: An Astronomical Web-Querying Package in Python
- Painting a portrait of the Galactic disc with its stellar clusters
- A catalog of newly identified star clusters in GAIA DR2
- Hunting for open clusters in \textit{Gaia} DR2: new OCs in the Galactic disc
- Improving the open cluster census. I. Comparison of clustering algorithms applied to Gaia DR2 data
- Extended stellar systems in the solar neighborhood - I. The tidal tails of the Hyades
- The extended halo of NGC 2682 (M 67) from Gaia DR2
- The Galactic metallicity gradient shown by open clusters in the light of radial migration
- Corona-Australis DANCe. I. Revisiting the census of stars with Gaia-DR2 data
- Exploring open cluster properties with Gaia and LAMOST
- Diagnosing the Stellar Population and Tidal Structure of the Blanco1 Star Cluster
- The substructure and halo population of the Double Cluster and Persei
- New Open Cluster candidates Found in Galactic Disk Using Gaia DR2/EDR3 Data
- Uncovering a 260 pc wide, 35 Myr old filamentary relic of star formation
- Extended main-sequence turnoffs in the double cluster and Persei: The complex role of stellar rotation
- Gaia-based Isochronal, Kinematic, and Spatial Analysis of the Cha Association
- How do binary clusters form?
- The list of possible double and multiple open clusters between galactic longitudes 240 and 270 degrees
- Multi-colour photometry and Gaia EDR3 astrometry of two couples of binary clusters (NGC 5617 and Trumpler 22) and (NGC 3293 and NGC 3324)
- Investigating Galactic binary cluster candidates with Gaia EDR3
- The substructure of the Perseus star forming region: A survey with Gaia DR2
- Discovery of extended structure around open cluster COIN-Gaia 13 based on Gaia EDR3
- Revisit of open clusters UPK 39, UPK 41 and PHOC 39 : a new binary open cluster found
Cited by in corpus (22)
- Improving the open cluster census. II. An all-sky cluster catalogue with Gaia DR3
- WIde Separation Planets In Time (WISPIT): A Gap-clearing Planet in a Multi-ringed Disk around the Young Solar-type Star WISPIT 2
- Using the Gaia excess uncertainty as a proxy for stellar variability and age
- Survey for Distant Stellar Aggregates in Galactic Disk: Detecting Two Thousand Star Clusters and Candidates, along with the Dwarf Galaxy IC10
- A study of newly discovered close binary open clusters in the Milky Way
- A fast-rotating blue straggler star in the tidal tail of the open cluster NGC 752
- Cluster aggregates surrounding Pismis 5 in the Vela Molecular Ridge
- Nearby open clusters with tidal features: golden sample selection and 3D structure
- Unveiling the Binary Nature of NGC 2323
- Star-by-star dynamical evolution of the physical pair of the Collinder 135 and UBC 7 open clusters
- Exploration of morphological coherence in open clusters with a "core-shell'' structure
- Open superclusters I: The most populated primordial groups of open clusters in the third quadrant of the Galactic disc
- Bayesian ages of local young stellar associations I. Through the expansion rate method
- Lost Sisters Found: TESS and Gaia Reveal a Dissolving Pleiades Complex
- Extended Main Sequences in Star Clusters
- On the Encounter Rate of Open Star Clusters
- Toward the fabric of the Milky Way I. The density of disk streams from a local pc volume
- LAMOST medium-resolution spectroscopic survey of Galactic Open Clusters (LAMOST-MRS-O): An overview of survey plan and preliminary results
- Mapping the reddening plane in the Galactic disk through interstellar extinction of open clusters
- Moving Groups in the Solar Neighborhood with Gaia, APOGEE, GALAH, and LAMOST: Dynamical Effects Gather Gas and the Ensuing Star Formation Plays an Important Role in Shaping the Stellar Velocity Distributions
- Missing pairs in open cluster catalogs
- Consensus based Algorithm for Nonparametric Detection of Star Clusters (CANDiSC)