financial support from the Russian Science Foundation (grant No.20-72-10052)。
We fit various color–magnitude diagrams(CMDs) of the high-latitude Galactic globular clusters NGC 5024(M53),NGC 5053,NGC 5272(M3),NGC 5466,and NGC 7099(M30) by isochrones from the Dartmouth Stellar Evolution Database...
supported by Yunnan Academician Workstation of Wang Jingxiu(202005AF150025);China Manned Space Project(NO.CMSCSST-2021-A08);Guanghe project(ghfund202302019167);the Natural Science Foundation of Yunnan Province(No.202201BC070003)。
Recent studies indicate that some Galactic open clusters(OCs)exhibit extended main-sequence turnoff(eMSTO)in their color–magnitude diagrams(CMDs).However,the number of Galactic OCs with eMSTO structures detected so f...
supported in part by China Manned Space Project with NO.CMS-CSST-2021-A08;the National Natural Science Foundation of China(NSFC,Grants Nos.12233009,12233013,12073090 and 12003001)。
The China Space Station Telescope(CSST)is a 2 m space-based optical-UV telescope.Its primary goal is to carry out a high-resolution photometric imaging survey of a 17,500 square degree sky area using the on board Surv...
the National Natural Science Foundation of China(No.11863002);Yunnan Academician Workstation of Wang Jingxiu(No.202005AF150025);Sino-German Cooperation Project(No.GZ 1284);Research Fund Project of Yunnan Education Department(Nos.2020J0545 and 2021J0335)。
We investigate the effects of binaries on the cluster age determination for 561 open clusters in the Galactic disk via the Bayesian statistical framework.Stellar properties of these star clusters,including age,metalli...
support through Grant Nos.11633005 and 12073090;the National Key R&D Program of China(Grant No.2020YFC2201400)。
Many evidences show that the Multiple Population(MP)features exist not only in old clusters but also in intermediate-age clusters in the Megallanic Clouds(MCs),which are characterized by star-to-star abundance scatter...
Funding for the DPAC has been provided by national institutions,in particular the institutions participating in the Gaia Multilateral Agreement.This research has made use of the VizieR catalogue access tool,CDS,Strasbourg,France(DOI:10.26093/cds/vizier).
The physical nature of a series of 20 new open clusters is confirmed employing existing data on putative star members,mainly from the second Gaia Data Release(DR2).The clusters were discovered as overdensities of star...
supported by the National Natural Science Foundation of China (Grant Nos. 11563002 and 11373003);the Joint Research Project of Sino-German Center (GZ1284);the National Key Basic Research Program of China (973 Program No. 2015CB857002);Yunnan Science Foundation (project name "Study of Binary Fraction of Star Clusters")
We present a new tool for color-magnitude diagram(CMD) studies, Powerful CMD. This tool is built based on the advanced stellar population synthesis(ASPS) model, in which single stars, binary stars, rotating stars ...
supported by the National Natural Science Foundation of China (NSFC, Grant No. 11403004)
We introduce a non-parametric method for open cluster membership determination in threedimensional(3D) velocity space(proper motion and radial velocity). Clean 3D cluster members can be obtained by statistically a...
supported by the National Natural Science Foundation of China(NSFC;Grant No.11403004);the School Foundation of Changzhou University(ZMF1002121);support by the 973 Program(2014 CB845702);the Strategic Priority Research Program"The Emergence of Cosmological Structures"of the Chinese Academy of Sciences(CAS;grant XDB09010100);the NSFC(Grant No.11373054)
In order to obtain clean members of the open cluster NGC 6819, the proper motions and radial velocities of 1691 stars are used to construct a three-dimensional (3D) velocity space. Based on the DBSCAN clustering alg...
supported by the National Natural Science Foundation of China(NSFC,Grant No.11403004);the School Foundation of Changzhou University(ZMF1002121);support by the 973 Program(2014CB845702);the Strategic Priority Research Program The Emergence of Cosmological Structures of the Chinese Academy of Sciences(CAS;grant XDB09010100);by the NSFC(No.11373054)
Abstract We report the discovery of 45 high-velocity extreme horizontal branch (EHB) stars in the globular cluster Omega Centauri (NGC 5139). The tangential ve- locities of these EHB stars are determined to be in ...