/ftp/cats/J_other/RAA/21.93



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J/other/RAA/21.93   74 new open clusters found in Gaia DR2           (He+, 2021)
The following files can be converted to FITS (extension .fit or fit.gz)
	new-oc.dat members.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/other/RAA/21.93
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drwxr-xr-x 91 cats archive 4096 Apr 16 16:21 [Up] drwxr-xr-x 3 cats archive 299 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 484 Nov 21 2022 .message -r--r--r-- 1 cats archive 5287 Nov 21 2022 ReadMe -rw-r--r-- 1 cats archive 1256 Nov 21 2022 +footg5.gif -rw-r--r-- 1 cats archive 4064 Nov 21 2022 +footg8.gif -r--r--r-- 1 cats archive 361158 Nov 21 2022 members.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 6142 Oct 28 2020 new-oc.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/other/RAA/21.93 74 new open clusters found in Gaia DR2 (He+, 2021) ================================================================================ A catalogue of 74 new open clusters found in Gaia Data-Release 2. He Z.-H., Xu Y., Hao C.-J., Wu Z.-Y., Li J.-J. <Res. Astron. Astrophys. 21, 93 (2021)> =2021RAA....21...93H (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Milky Way ; Clusters, open ; Proper motions ; Optical Keywords: Galaxy: open clusters - methods: data analysis - surveys Abstract: Based on astrometric data from Gaia Data-Release 2 (DR2), we employ an un- supervised machine learning method to blindly search for open star clusters in the Milky Way within the Galactic latitude range of |b|<20degree. In addition to 2080known clusters, 74 new open cluster candidates are found. In this work, we present the positions, apparent radii, parallaxes, proper motions and member stars of these candidates. Meanwhile, to obtain the physical parameters of each candidate cluster, stellar isochrones are fit to the photometric data. The results show that the apparent radii and the observed proper motion dispersions of these new candidates are consistent with those of open clusters previously identified in Gaia DR2. Description: Adopting the clustering algorithm DBSCAN, we used the positions, parallaxes, and proper motions of nearly 170 million stars within the galactic latitude range |b|<20deg and parallax plx>0.2mas in Gaia DR2 to search for unknown OCs. We cross-matched our initial sample with previous star cluster catalogues, and after performing several vetting stages, we obtained a catalogue of 74 new OC candidates. We fitted isochrones to these candidates and obtained their corresponding physical parameters. The apparent radii and observed proper motion dispersions of the new cluster candidates were consistent with those of OCs previously found in Gaia DR2.