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相关论文: Old open clusters: UBGVRI photometry of NGC 2506

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We present UBVRI photometry for the old open cluster NGC 6253. From comparison of the observed colour-magnitude diagrams with simulations based on stellar evolutionary models we derive in a self consistent way reddening, distance, and age…

天体物理学 · 物理学 2015-06-24 A. Bragaglia , G. Tessicini , M. Tosi , G. Marconi , U. Munari

We present UBVI photometry for the old open cluster Collinder 261. From comparison of the observed colour-magnitude diagrams with simulations based on stellar evolutionary models we derive in a self consistent way reddening, distance, and…

天体物理学 · 物理学 2015-06-24 E. Gozzoli , M. Tosi , G. Marconi , A. Bragaglia

We present CCD UBVI photometry of the intermediate old open cluster NGC2660, covering from the red giants region to about seven magnitudes below the main sequence turn-off. Using the synthetic Colour - Magnitude Diagram method, we estimate…

天体物理学 · 物理学 2009-10-31 S. Sandrelli , A. Bragaglia , M. Tosi , G. Marconi

We present CCD UBVI photometry of the nearby, intermediate age open cluster NGC 6939. Using the synthetic Colour - Magnitude Diagrams technique we estimate the following parameters: age between 1.3 and 1.0 Gyr (depending on whether or not…

天体物理学 · 物理学 2009-11-10 Gloria Andreuzzi , Angela Bragaglia , Monica Tosi , Gianni Marconi

Using high-precision observations from the space-based \textit{Gaia} and \textit{TESS} missions, complemented by ground-based spectroscopic data and multi-band photometric surveys, we perform a detailed investigation of the Galactic open…

太阳与恒星天体物理 · 物理学 2025-10-09 K. Yakut , B. Kalomeni , S. Rappaport , Veselin Kostov

Precision uvbyCa Hbeta photometry of the metal-deficient, old open cluster, NGC 2506, is presented. The survey covers an area 20 by 20 arcminutes, and extends to V~18 for b-y and Hbeta and to V~17.0 for c_1 and hk. For V < 16.0, photometric…

太阳与恒星天体物理 · 物理学 2016-12-07 B. J. Anthony-Twarog , C. P. Deliyannis , B. A. Twarog

We report on $BVI$ CCD photometry of a field centered on the region of the intermediate-age open cluster NGC 2112 down to V=21. Due to the smaller field coverage, we are able to limit the effect of field star contamination which hampered in…

天体物理学 · 物理学 2009-11-07 Giovanni Carraro , Roberto Barbon , Carla S. Boschetti

Accurate stellar parameters of stars in open clusters can help constrain models of stellar structure and evolution. Here we wish to determine the age and metallicity content of the open cluster NGC 2506. To this end we investigated three…

The fundamental parameters of reddening, metallicity, age, and distance are presented for the poorly studied open clusters Be~89, Ru~135, and Be~10, derived from their CCD UBVRI photometry. By fitting the appropriate isochrones to the…

The open clusters NGC 2323 and NGC 2539 have been analysed using CCD UBV(RI)KC photometric data, observed at the San Pedro Martir Observatory. Cluster memberships have been determined with the proper motion and parallax measures from the…

$UBVRI$ photometry of the five open clusters Czernik 4, Berkeley 7, NGC 2236, NGC 7226 and King 12 has been carried out using ARIES 104 cm telescope, Nainital. Fundamental cluster parameters such as foreground reddening $E(B-V)$, distance,…

太阳与恒星天体物理 · 物理学 2015-06-16 Sneh Lata , A. K. Pandey , Saurabh Sharma , Charles Bonatto , Ram Kesh Yadav

We present the $UBVRI$ CCD photometry in the region of the open cluster NGC 2421. Radius of the cluster is determined as $\sim$ 3$^\prime$.0 using stellar density profile. Our Study indicates that metallicity of the cluster is $Z \sim$…

天体物理学 · 物理学 2009-11-10 R. K. S. Yadav , Ram Sagar

We present UBVRI photometry for the young open cluster NGC 2362. From analysis of the appropriate color-color and color-magnitude diagrams we derive the fundamental parameters of the NGC 2362 cluster to be: age = 5 (+1-2) Myr, distance =…

天体物理学 · 物理学 2009-11-07 A. Moitinho , J. Alves , N. Huelamo , C. Lada

NGC 663 is a young, moderately rich open cluster, known to contain one of the largest fractions of Be stars among all galactic clusters. In this work we present CCD uvby-beta photometry for stars in its central area. We have used these data…

天体物理学 · 物理学 2009-11-10 J. Fabregat , G. Capilla

We present a robust methodology for identifying photometric binaries in star clusters. Using Gaia DR3, Pan-STARRS and 2MASS data, we self-consistently define the cluster parameters and binary demographics for the open clusters (OCs) NGC…

太阳与恒星天体物理 · 物理学 2023-12-22 Anna C. Childs , Aaron M. Geller , Ted von Hippel , Erin Motherway , Claire Zwicker

We report on $UBVRI$ CCD photometry of two overlapping fields in the region of the intermediate-age open cluster NGC 2158 down to V=21. By analyzing Colour-Colour (CC) and Colour-Magnitude Diagrams (CMD) we infer a reddening $E_{B-V}=…

天体物理学 · 物理学 2016-08-30 Giovanni Carraro , Leo Girardi , Paola Marigo

We present UBVI photometry of the old open cluster NGC 1193. Color-magnitude diagrams (CMDs) of this cluster show a well defined main sequence and a sparse red giant branch. For the inner region of r<50 arcsec, three blue straggler…

天体物理学 · 物理学 2015-05-13 Jaemann Kyeong , Sang Chul Kim , David Hiriart , Eon-Chang Sung

We have conducted VI CCD photometry of the two open clusters NGC 1245 and NGC 2506 using the CFH12K CCD camera. Our photometry covers a sky area of 84'X82' and 42'X81' for the two clusters, respectively, and reaches down to V = 23. We…

星系天体物理 · 物理学 2015-06-11 S. H. Lee , Y. -W. Kang , H. B. Ann

We present UBVI CCD photometry of two open clusters NGC 1798 and NGC 2192 which were little studied before. Color-magnitude diagrams of these clusters show several features typical for old open clusters: a well-defined main-sequence, a red…

天体物理学 · 物理学 2007-05-23 Hong Soo Park , Myung Gyoon Lee

We report on CCD optical (B and V passbands) and near IR (J and K bands) observations in the region of the old open cluster NGC 2141. By combining the two sets of photometry (500 stars in common) we derive new estimates of the cluster…

天体物理学 · 物理学 2009-11-06 G. Carraro , S. Hassan , S. Ortolani , A. Vallenari
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