Cl Berkeley 67 , the SIMBAD biblio

Cl Berkeley 67 , the SIMBAD biblio (34 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST07:38:15

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1966BAICz..17...33R 319 154 Classification of open star clusters. RUPRECHT J.
2004BASI...32...59L 73 T                   3 5 CCD photometry of the unstudied galactic star clusters Be 10,
Be 67 and To 5. 		LATA S., MOHAN V., PANDEY A.K., et al.
2005BASI...33...51L 73 T                   7 2 Mass function study of six open clusters Be 10,
Be 67, To 5, Be 15, Be 71 and King 1. 		LATA S.
2005BASI...33..377L 73 T                   6 0 Mass function study of six open clusters Be 10,
Be 67, To 5, Be 15, Be 71 and King 1. 		LATA S. and SAGAR R.
2007A&A...467.1065M 274       D     X C       7 43 102 CCD BV survey of 42 open clusters. MACIEJEWSKI G. and NIEDZIELSKI A.
2012A&A...543A.156K viz 15       D               1 657 80 Global survey of star clusters in the Milky Way. I. The pipeline and fundamental parameters in the second quadrant. KHARCHENKO N.V., PISKUNOV A.E., SCHILBACH E., et al.
2013MNRAS.436.1465B viz 15       D               1 779 10 Properties of star clusters - I. Automatic distance and extinction estimates. BUCKNER A.S.M. and FROEBRICH D.
2013A&A...558A..53K viz 15       D               1 3009 561 Global survey of star clusters in the Milky Way. II. The catalogue of basic parameters. KHARCHENKO N.V., PISKUNOV A.E., SCHILBACH E., et al.
2014A&A...564A..79D viz 15       D               1 1795 136 Proper motions of the optically visible open clusters based on the UCAC4 catalog. DIAS W.S., MONTEIRO H., CAETANO T.C., et al.
2014MNRAS.444..290B viz 15       D               1 300 28 Properties of star clusters - II. Scaleheight evolution of clusters. BUCKNER A.S.M. and FROEBRICH D.
2016A&A...585A.101K viz 16       D               1 3071 67 Global survey of star clusters in the Milky Way. V. Integrated JHKS magnitudes and luminosity functions. KHARCHENKO N.V., PISKUNOV A.E., SCHILBACH E., et al.
2017MNRAS.470.3937S viz 16       D               1 1853 51 A multimembership catalogue for 1876 open clusters using UCAC4 data. SAMPEDRO L., DIAS W.S., ALFARO E.J., et al.
2018AJ....155...91Y viz 16       D               1 133 2 Searching for Be stars in the open clusters with PTF/iPTF. I. Cluster sample and Be star candidates. YU P.-C., YU C.-H., LEE C.-D., et al.
2018A&A...618A..93C viz 16       D               1 87620 517 A Gaia DR2 view of the open cluster population in the Milky Way. CANTAT-GAUDIN T., JORDI C., VALLENARI A., et al.
2018A&A...619A.155S viz 16       D               1 875 129 Open cluster kinematics with Gaia DR2. SOUBIRAN C., CANTAT-GAUDIN T., ROMERO-GOMEZ M., et al.
2019ApJS..245...32L viz 16       D               2 1259 127 A catalog of newly identified star clusters in Gaia DR2. LIU L. and PANG X.
2020A&A...633A..99C viz 16       D               1 257585 169 Clusters and mirages: cataloguing stellar aggregates in the Milky Way. CANTAT-GAUDIN T. and ANDERS F.
2020MNRAS.495.2882S viz 16       D               1 404 ~ A catalogue of open cluster radii determined from Gaia proper motions. SANCHEZ N., ALFARO E.J. and LOPEZ-MARTINEZ F.
2020A&A...640A...1C viz 16       D               1 235399 241 Painting a portrait of the Galactic disc with its stellar clusters. CANTAT-GAUDIN T., ANDERS F., CASTRO-GINARD A., et al.
2020A&A...640A.127Z viz 16       D               1 9108 33 Exploring open cluster properties with Gaia and LAMOST. ZHONG J., CHEN L., WU D., et al.
2021A&A...647A..19T viz 17       D               1 24814 55 3D kinematics and age distribution of the open cluster population. TARRICQ Y., SOUBIRAN C., CASAMIQUELA L., et al.
2021MNRAS.503..236J viz 878   K A D     X C       21 8100 9 UOCS - III. UVIT catalogue of open clusters with machine learning-based membership using Gaia EDR3 astrometry. JADHAV V.V., PENNOCK C.M., SUBRAMANIAM A., et al.
2021MNRAS.504..356D viz 17       D               1 1748 88 Updated parameters of 1743 open clusters based on Gaia DR2. DIAS W.S., MONTEIRO H., MOITINHO A., et al.
2021A&A...651A.104P viz 17       D               1 1886 63 Galactic spiral structure revealed by Gaia EDR3. POGGIO E., DRIMMEL R., CANTAT-GAUDIN T., et al.
2021MNRAS.507.1699J viz 17       D               1 2039 15 Blue straggler stars in open clusters using Gaia: dependence on cluster parameters and possible formation pathways. JADHAV V.V. and SUBRAMANIAM A.
2021A&A...656A..49H viz 17       D               1 1256 6 Decoding the morphological evolution of open clusters. HU Q., ZHANG Y. and ESAMDIN A.
2022A&A...663A..39B 85             C       1 146 6 The origin of early-type runaway stars from open clusters. BHAT A., IRRGANG A. and HEBER U.
2022A&A...668A...4F viz 17       D               1 4599 5 LAMOST meets Gaia: The Galactic open clusters. FU X., BRAGAGLIA A., LIU C., et al.
2023A&A...672A.187J viz 17       D               1 2885 1 Global survey of star clusters in the Milky Way VII. Tidal parameters and mass function. JUST A., PISKUNOV A.E., KLOS J.H., et al.
2023A&A...674A..37G viz 17       D               1 5822 41 Gaia Data Release 3 Mapping the asymmetric disc of the Milky Way. GAIA COLLABORATION, DRIMMEL R., ROMERO-GOMEZ M., et al.
2023ApJS..268...46L viz 17       D               1 4895 ~ Kinematics of the Local Spiral Structure Revealed by Young Stars in Gaia DR3. LIU D., XU Y., HAO C., et al.
2024A&A...684A.109C 45           X         1 31 ~ Mass density profiles at kiloparsec scales using the sub-millimetre galaxies magnification bias. CRESPO D., GONZALEZ-NUEVO J., BONAVERA L., et al.
2024ApJS..275...34P viz 63       D     X         2 37 ~ A Comprehensive Catalog of UVIT Observations. I. Catalog Description and First Release of Source Catalog (UVIT DR1). PIRIDI S., KUMAR R., PANDEY D., et al.
2025A&A...693A.305A viz 19       D               1 1726 ~ Open cluster dissolution rate and the initial cluster mass function in the solar neighbourhood Modelling the age and mass distributions of clusters observed by Gaia. ALMEIDA D., MOITINHO A. and MOREIRA S.

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