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
New and existing X-ray, UBVJHKsW(1−4), and spectroscopic observations were analyzed to constrain fun...
Open clusters are convenient probes of the structure and history of the Galactic disk. They are also...
Context. The improvements in the precision of the published data in Gaia EDR3 with respect to Gaia D...
The latest Gaia Data Release 3 provides an opportunity to expand the census of Galactic open cluster...
The latest Gaia Data Release 3 provides an opportunity to expand the census of Galactic open cluster...
Classical Cepheids in open clusters are valuable ingredients for studies concerning young stellar po...
We analyse all potential combinations of Galactic Cepheids and open clusters (OCs) in the most up-to...
Classical Cepheids in open clusters play an important role in benchmarking stellar evolution models,...
Classical Cepheids are crucial calibrators of the extragalactic distance scale. Despite the adjectiv...
International audienceContext. Open clusters (OCs) are popular tracers of the structure and evolutio...
We report 541 new open cluster candidates in Gaia EDR3 through revisiting the cluster results from a...
Context. Open clusters (OCs) are popular tracers of the structure and evolutionary history of the Ga...
New and existing X-ray, UBVJHKsW(1 - 4), and spectroscopic observations were analyzed to constrain f...
[Context] The improvements in the precision of the published data in Gaia EDR3 with respect to Gaia ...
We investigate the reddening and Main Sequence fitted distances to elevenyoung, Galactic open cluste...
New and existing X-ray, UBVJHKsW(1−4), and spectroscopic observations were analyzed to constrain fun...
Open clusters are convenient probes of the structure and history of the Galactic disk. They are also...
Context. The improvements in the precision of the published data in Gaia EDR3 with respect to Gaia D...
The latest Gaia Data Release 3 provides an opportunity to expand the census of Galactic open cluster...
The latest Gaia Data Release 3 provides an opportunity to expand the census of Galactic open cluster...
Classical Cepheids in open clusters are valuable ingredients for studies concerning young stellar po...
We analyse all potential combinations of Galactic Cepheids and open clusters (OCs) in the most up-to...
Classical Cepheids in open clusters play an important role in benchmarking stellar evolution models,...
Classical Cepheids are crucial calibrators of the extragalactic distance scale. Despite the adjectiv...
International audienceContext. Open clusters (OCs) are popular tracers of the structure and evolutio...
We report 541 new open cluster candidates in Gaia EDR3 through revisiting the cluster results from a...
Context. Open clusters (OCs) are popular tracers of the structure and evolutionary history of the Ga...
New and existing X-ray, UBVJHKsW(1 - 4), and spectroscopic observations were analyzed to constrain f...
[Context] The improvements in the precision of the published data in Gaia EDR3 with respect to Gaia ...
We investigate the reddening and Main Sequence fitted distances to elevenyoung, Galactic open cluste...
New and existing X-ray, UBVJHKsW(1−4), and spectroscopic observations were analyzed to constrain fun...
Open clusters are convenient probes of the structure and history of the Galactic disk. They are also...
Context. The improvements in the precision of the published data in Gaia EDR3 with respect to Gaia D...