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相关论文: Intermediate age open clusters: Collinder 110

200 篇论文

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 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

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 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…

天体物理学 · 物理学 2009-11-07 L. Di Fabrizio , 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

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…

天体物理学 · 物理学 2009-11-13 A. Bragaglia , M. Tosi , E. Carretta , R. G. Gratton , G. Marconi , E. Pompei

We present BV CCD photometry for the open clusters Czernik 24 and Czernik 27. These clusters have never been studied before, and we provide, for the first time, the cluster parameters; reddening, distance, metallicity and age. Czernik 24 is…

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…

天体物理学 · 物理学 2007-05-23 Annapurni Subramaniam

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…

天体物理学 · 物理学 2007-05-23 Antonella Vallenari , Giovanni Carraro , Andrea Richichi

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 analyzed HST/WFPC2 colour-magnitude diagrams (CMDs) of 15 populous Large Magellanic Cloud (LMC) stellar clusters with ages between ~ 0.3 Gyr and ~ 3 Gyr. These (V, B-V) CMDs are photometrically homogeneous and typically reach V \~ 22.…

天体物理学 · 物理学 2009-11-11 L. O. Kerber , B. X. Santiago , E. Brocato

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

Fundamental astrophysical parameters have been derived for 20 open clusters (O\!Cs) using CCD~$U\!BV\!(RI)_C$ photometric data observed with the 84~cm telescope at the San Pedro M\'artir National Astronomical Observatory, M\'exico. The…

星系天体物理 · 物理学 2015-06-22 Inci Akkaya Oralhan , Yüksel Karataş , William J. Schuster , Raúl Michel , Carlos Chavarría

In this paper we study the properties of ten halo globular clusters in the nearby spiral galaxy M33. CCD images of M33 were obtained as a part of the BATC Colour Survey of the sky in 13 intermediate-band filters from 3800 to 10000{\AA}. By…

天体物理学 · 物理学 2009-11-07 Jun Ma , Xu Zhou , Jiansheng Chen , Hong Wu , Zhaoji Jiang , Suijian Xue , Jin Zhu

The LMC has a rich star cluster system spanning a wide range of ages and masses. One striking feature of the LMC cluster system is the existence of an age gap between 3-10 Gyrs. But this feature is not as clearly seen among field stars.…

宇宙学与河外天体物理 · 物理学 2015-05-18 E. Balbinot , B. X. Santiago , L. O. Kerber , B. Barbuy , B. M. S. Dias

CCD photometry on the intermediate-band uvbyCa H beta system is presented for the anticenter, intermediate-age open cluster, Melotte 71. Restricting the data to probable single members of the cluster using the color-magnitude diagram and…

天体物理学 · 物理学 2008-11-26 B. A. Twarog , S. Corder , B. J. Anthony-Twarog

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

We report on near IR (J and K bands) observations of an $8^{\prime} \times 8^{\prime}$ region centered on the poorly studied open cluster King 5, for which only optical photometry existed. We found that the cluster is of moderate age (1.0…

天体物理学 · 物理学 2009-10-31 Giovanni Carraro , Antonella Vallenari

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…

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