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Related papers: The intermediate age open cluster NGC 2660

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UBGVRI photometry for the open cluster NGC 2506 is presented. 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 of…

Astrophysics · Physics 2015-06-24 G. Marconi , D. Hamilton , M. Tosi , A. Bragaglia

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}=…

Astrophysics · Physics 2016-08-30 Giovanni Carraro , Leo Girardi , Paola Marigo

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…

Astrophysics · Physics 2009-11-10 Gloria Andreuzzi , Angela Bragaglia , Monica Tosi , Gianni Marconi

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…

Astrophysics · Physics 2009-11-07 Giovanni Carraro , Roberto Barbon , Carla S. Boschetti

We present CCD UBVI photometry and high-resolution spectroscopy of the intermediate age open cluster NGC 3960. The colour - magnitude diagrams (CMDs) derived from the photometric data and interpreted with the synthetic CMD method allow us…

Astrophysics · Physics 2009-11-13 A. Bragaglia , M. Tosi , E. Carretta , R. G. Gratton , G. Marconi , E. Pompei

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…

Astrophysics · Physics 2015-06-24 A. Bragaglia , G. Tessicini , M. Tosi , G. Marconi , U. Munari

We present CCD BV photometry of the intermediate age open cluster Collinder 110, a nearby, scarcely populated, and poorly studied system. There is no literature information on the metallicity, so we tested several possibilities, and found a…

Astrophysics · Physics 2009-11-07 Angela Bragaglia , Monica Tosi

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…

Astrophysics · Physics 2015-06-24 E. Gozzoli , M. Tosi , G. Marconi , A. Bragaglia

We present the first $BVI$ CCD photometry to $V=22.0$ of 4 fields centered on the region of the southern Galactic star clusters Ruprecht~61, Czernik~32, NGC 2225 and NGC 2262 and of 4 displaced control fields. These clusters were never…

Astrophysics · Physics 2009-11-13 G. Carraro , G. Baume , R. Vazquez , A. Moitinho , D. Geisler

We present CCD BVI photometry of the intermediate age open cluster Pismis 2, covering from the brighter red giants to about 5 magnitudes below the main sequence turn-off. The cluster is heavily reddened and is possibly affected by a…

Astrophysics · Physics 2009-11-07 L. Di Fabrizio , A. Bragaglia , M. Tosi , G. 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…

Solar and Stellar Astrophysics · Physics 2025-10-09 K. Yakut , B. Kalomeni , S. Rappaport , Veselin Kostov

The B,V CCD photometry of 916 stars in the field of the high galactic latitude intermediate age open cluster NGC 1245 is presented. The cluster parameters were estimated with the help of V vs (B-V) colour-magnitude diagram (CMD). After…

Astrophysics · Physics 2007-05-23 Annapurni Subramaniam

We analyse CCD broad band (UBV(RI)c) photometric data obtained in the fields of the poorly studied open clusters NGC 2425 and NGC 2635. Both clusters are found to be of intermediate age thus increasing the population of open clusters known…

Astrophysics · Physics 2009-11-11 A. Moitinho , G. Carraro , G. Baume , R. A. Vazquez

We present UBV CCD observations obtained in the field of the northern open cluster NGC 1220, for which little information is available. We provide also BV CCD photometry of a field 5$^{\prime}$ northward of NGC 1220 to take into account…

Astrophysics · Physics 2009-11-07 S. Ortolani , G. Carraro , S. Covino , E. Bica , B. Barbuy

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…

Astrophysics · Physics 2009-11-10 J. Fabregat , G. Capilla

We present BVI photometry for poorly known southern hemisphere open clusters: NGC 2425, Haffner 10 and Czernik 29. We have calculated the density profile and established the number of stars in each cluster. The colour-magnitude diagrams of…

Astrophysics · Physics 2009-11-13 P. Pietrukowicz , J. Kaluzny , W. Krzeminski

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…

Astrophysics · Physics 2015-05-13 Jaemann Kyeong , Sang Chul Kim , David Hiriart , Eon-Chang Sung

We present deep CCD BVI photometry of the distant, old open cluster Berkeley 22, covering from the red giants branch (RGB) to about 6 magnitudes below the main sequence (MS) turn-off. Using the synthetic Colour - Magnitude Diagram method…

Astrophysics · Physics 2009-11-10 L. Di Fabrizio , A. Bragaglia , M. Tosi , G. Marconi

We present and discuss new photometric data obtained with an IR camera in the J and K pass-bands for the intermediate age open clusters IC 166 (936 stars in total) and NGC 7789 (1030 stars in total). Ic 166 is a poorly studied open cluster…

Astrophysics · Physics 2007-05-23 Antonella Vallenari , Giovanni Carraro , Andrea Richichi

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 $Z \sim$…

Astrophysics · Physics 2009-11-10 R. K. S. Yadav , Ram Sagar
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