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相关论文: Investigating kinematics and dynamics of three ope…

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In this study, we present a comprehensive analysis of the structural, astrophysical, and dynamical properties of eight open clusters: NGC 559, NGC 1817, NGC 2141, NGC 7245, Ruprecht 15, Ruprecht 137, Ruprecht 142, and Ruprecht 169, using…

星系天体物理 · 物理学 2026-02-04 A. Ahmed , W. H. Elsanhoury , D. C. Çınar , A. A. Haroon , M. S. Alenazi , E. A. Alkholy

In this paper, we present astrophysical parameters of the open cluster King 13 based on the VI CCD and 2MASS JHKs photometric data. This is a poorly studied cluster, for which new results have been found in the present work. To identify…

星系天体物理 · 物理学 2020-02-12 Alok Durgapal , D Bisht , Geeta Rangwal , Harmeen Kaur , R. K. S. Yadav

We present a kinematic and dynamical analysis of six Galactic open clusters NGC~2204, NGC~2660, NGC~2262, Czernik~32, Pismis~18, and NGC~2437, using \textit{Gaia}~DR3. We used Bayesian and Gaussian Mixture Model (GMM) methods to identify…

In this paper we analyse the evolutionary status and properties of the old open cluster NGC 2355, located in the Galactic anticentre direction, as a part of the long term programme BOCCE. NGC 2355 was observed with LBC@LBT using the Bessel…

太阳与恒星天体物理 · 物理学 2015-09-30 P. Donati , A. Bragaglia , E. Carretta , V. D'Orazi , M. Tosi , F. Cusano , R. Carini

NGC 2355 is an old open cluster in the outer part of the galactic disk (l=203 deg, b=+11 deg) which has been little studied until now. This paper presents the first astrometric and spectroscopic investigation of this cluster. We have…

天体物理学 · 物理学 2007-05-23 C. Soubiran , M. Odenkirchen , J. -F. Le Campion

We present the dynamical evolution of ten open clusters which were part of our previous studies. These clusters include both young and intermediate-age open clusters with ages ranging from 25$\pm$19 Myr to 1.78$\pm$0.20 Gyr. The total mass…

星系天体物理 · 物理学 2023-07-19 Jayanand Maurya , Y. C. Joshi , Manash Ranjan Samal , Vineet Rawat , Anubha Singh Gour

We present photometric, astrometric, and kinematic studies of the old open star clusters NGC 1193 and NGC 1798. Both of the clusters are investigated by combining data sets from Gaia EDR3 and CCD UBV observational data. Analysis of the…

星系天体物理 · 物理学 2022-10-12 T. Yontan , H. Cakmak , S. Bilir , T. Banks , M. Raul , R. Canbay , S. Koc , S. Tasdemir , H. Ercay , B. Tanik Ozturk , D. C. Dursun

In this study, we carried out CCD UBV photometry of eight open clusters, ASCC 115, Collinder 421, NGC 6793, NGC 7031, NGC 7039, NGC 7086, Roslund 1, Stock 21, and determined their reddening, metallicity, distance, age, and mass functions.…

星系天体物理 · 物理学 2019-09-25 T. Yontan , S. Bilir , Z. F. Bostanci , T. Ak , S. Ak , T. Guver , E. Paunzen , H. Urgup , M. Celebi , B. A. Akti , S. Gokmen

A detailed analysis of ground-based CCD UBV photometry and space-based Gaia Data Release 3 (DR3) data for the open clusters King 6 and NGC 1605 was performed. Using the pyUPMASK algorithm on Gaia astrometric data to estimate cluster…

星系天体物理 · 物理学 2023-11-02 S. Gokmen , Z. Eker , T. Yontan , S. Bilir , T. Ak , S. Ak , T. Banks , A. Sarajedini

This paper investigates a poorly studied open cluster, NGC 5288, using 2MASS JHKS and the recently released Gaia DR3 astrometric and photometric data. The mean proper motions in Right Ascension and Declination are estimated as (-3.840 +/-…

星系天体物理 · 物理学 2023-05-18 Ritika Sethi , D. Bisht , Geeta Rangwal , A. Raj

We present a comprehensive analysis of four young open clusters, NGC 663, NGC 2301, NGC 2384, and NGC 7510, utilizing high-precision astrometric and photometric data from Gaia DR3. Cluster membership was determined using the UPMASK…

星系天体物理 · 物理学 2026-01-05 W. H. Elsanhoury , S. Taşdemir , D. C. Çınar , R. Canbay , A. A. Haroon , A. Ahmed

We have measured the absolute proper motions of four low-latitude, inner-Galaxy globular clusters. These clusters are: NGC 6266 (M62), NGC 6304, NGC 6316 and NGC 6723. The proper motions are on the Hipparcos system, as no background…

天体物理学 · 物理学 2009-11-07 Dana I. Dinescu , Terrence M. Girard , William F. van Altena , Carlos Lopez

This study reports the first comprehensive astrometric, photometric and kinematical analysis of four newly discovered open clusters; namely QC1, QC2, QC3, and QC4, using astrometric and photometric data from the most recent Gaia EDR3 for…

太阳与恒星天体物理 · 物理学 2022-05-25 W. H. Elsanhoury , Magdy Y. Amin , A. A. Haroon , Z. Awad

We derive fundamental parameters for the old, rich open cluster NGC 1245 using BVI photometry from the MDM 1.3m and 2.4m telescopes. Based on detailed isochrone fitting, we find NGC 1245 has a slightly sub-solar metallicity, [Fe/H]=-0.05 +-…

天体物理学 · 物理学 2009-11-10 Christopher J. Burke , B. Scott Gaudi , D. L. DePoy , Richard W. Pogge , Marc H. Pinsonneault

In the context of a project aimed at characterizing the properties of star clusters in the Galactic bulge, here we present the determination of the internal kinematics and structure of the massive globular cluster NGC 6569. The kinematics…

We present an analysis of three southern open star clusters NGC 6067, NGC 2506 and IC 4651 using wide-field photometric and Gaia DR2 astrometric data. They are poorly studied clusters. We took advantage of the synergy between Gaia DR2 high…

星系天体物理 · 物理学 2019-10-02 Geeta Rangwal , R. K. S. Yadav , Alok Durgapal , D. Bisht , D. Nardiello

This paper presents an investigation of an old age open cluster King 11 using Gaia's Early Data Release 3 (EDR3) data. Considering the stars with membership probability ($P_{\mu}$) $> 90\%$, we identified 676 most probable cluster members…

Luminosity and mass functions in the old open cluster NGC 188 are analysed by means of J and H 2MASS photometry. Within the uncertainties, the observed projected radial density profile of NGC 188 departs from the two-parameter King model in…

天体物理学 · 物理学 2009-11-10 C. Bonatto , E. Bica , J. F. C. Santos

We conducted a photometric and kinematic analysis of the young open cluster NGC 2345 using CCD \emph{UBV} data from 2-m Himalayan Chandra Telescope (HCT), \emph{Gaia} Data Release 3 (DR3), 2MASS, and the APASS datasets. We found 1732 most…

Aims: We present the first in-depth study of the kinematic properties and derive the structural parameters of NGC 4372 based on the fit of a Plummer profile and a rotating, physical model. We explore the link between internal rotation to…

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