Issue |
A&A
Volume 668, December 2022
|
|
---|---|---|
Article Number | A13 | |
Number of page(s) | 13 | |
Section | Catalogs and data | |
DOI | https://doi.org/10.1051/0004-6361/202244570 | |
Published online | 30 November 2022 |
Open clusters housing classical Cepheids in Gaia DR3★
1
Purple Mountain Observatory, Chinese Academy of Sciences,
Nanjing
210023, PR China
e-mail: xuye@pmo.ac.cn
2
School of Astronomy and Space Science, University of Science and Technology of China,
Hefei
230026, PR China
3
National Astronomical Observatories, Chinese Academy of Sciences,
20A Datun Road, Chaoyang District,
Beijing
100101, PR China
4
School of Astronomy and Space Science, University of Chinese Academy of Sciences,
Beijing
101408, PR China
Received:
22
July
2022
Accepted:
23
September
2022
The latest Gaia Data Release 3 provides an opportunity to expand the census of Galactic open clusters harboring classical Cepheid variables, thereby bolstering the cosmic distance scale. A comprehensive analysis yielded a total of 50 classical Cepheids associated with 45 open clusters, of which 39 open cluster-classical Cepheid pairs are considered probable, with the remaining 11 pairs considered improbable but worth following up. Two previously identified clusters by us possibly host classical Cepheids (OC-0125/V1788 Cyg and OC-0675/OGLE-BLG-CEP-114). In addition, we identify 38 new open cluster candidates within the Galactic disk.
Key words: Galaxy: stellar content / open clusters and associations: general / stars: variables: Cepheids / methods: data analysis
Data are only available at the CDS via anonymous ftp to cdsarc.cds.unistra.fr (130.79.128.5) or via https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/668/A13
© C. J. Hao et al. 2022
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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