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相关论文: Fundamental parameters of six neglected old open c…

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CCD BVI photometry of the faint open clusters Berkeley~73, Berkeley~75 and Berkeley~25 are presented. The two latter are previously unstudied clusters to our knowledge. While Berkeley~73 is found to be of intermediate-age (about 1.5 Gyr…

天体物理学 · 物理学 2009-11-11 G. Carraro , D. Geisler , A. Moitinho , G. Baume , R. Vazquez

We present BVI CCD photometry of 10 northern open clusters, Berkeley 43, Berkeley 45, Berkeley 47, NGC 6846, Berkeley 49, Berkeley 51, Berkeley 89, Berkeley 91, Tombaugh 4 and Berkeley 9, and estimate their fundamental parameters. Eight of…

星系天体物理 · 物理学 2015-05-18 Annapurni Subramaniam , Giovanni Carraro , Kenneth A. Janes , ;

New photometric material is presented for 6 outer disk supposedly old, Galact ic star clusters: Berkeley 76, Haffner 4, Ruprecht 10, Haffner 7, Haffner 11, and Haffner 15, that are projected against the rich and complex Canis Major overde…

星系天体物理 · 物理学 2015-06-11 Giovanni Carraro , Yuri Beletsky , Gianni Marconi

Photometric UBVI CCD photometry is presented for NGC 188 and Berkeley 17. Color-magnitude diagrams (CMDs) are constructed and reach well past the main-sequence turn-off for both clusters. Cluster ages are determined by means of isochrone…

天体物理学 · 物理学 2008-11-26 Zosia A. C. Krusberg , Brian Chaboyer

We have obtained BVI CCD imaging of Berkeley 17, an anticentre open cluster that competes with NGC 6791 as the oldest known open cluster. Using the synthetic colour magnitude diagrams (CMD) technique with three sets of evolutionary tracks…

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

We have obtained CCD UBVI_{KC} photometry down to V ~ 21.0 for the open clusters Berkeley 26, Czernik 27, Melotte 72, NGC 2479 and BH 37. The latter has never been studied before. Cluster stellar density profiles were obtained from star…

星系天体物理 · 物理学 2015-05-14 Andres E. Piatti , Juan J. Claria , Andrea V. Ahumada

In this paper we present the investigation of the evolutionary status of three open clusters: Berkeley 27, Berkeley 34, and Berkeley 36, all located in the Galactic anti-centre direction. All of them were observed with SUSI2@NTT using the…

星系天体物理 · 物理学 2015-06-05 P. Donati , A. Bragaglia , M. Cignoni , G. Cocozza , M. Tosi

We present CCD BVI photometry of the old open cluster Berkeley 21, one of the most distant clusters in the Galactic anticentre direction, and possibly the lowest metallicity object in the open clusters sample. Its position and metal…

天体物理学 · 物理学 2009-10-30 M. Tosi , L. Pulone , G. Marconi , A. Bragaglia

We present CCD BVI photometry of the old open cluster Berkeley 29, located in the anticentre direction. Using the synthetic Colour - Magnitude Diagrams technique we estimate at the same time its age, reddening, distance, and approximate…

天体物理学 · 物理学 2009-11-10 M. Tosi , L. Di Fabrizio , A. Bragaglia , P. A. Carusillo , G. Marconi

CCD $BVI$ photometry is presented for 8 previously unstudied star clusters located in the First and Fourth Galactic Quadrants: AL~1, BH 150, NGC 5764, Lynga~9, Czernik~37, BH 261, Berkeley~80 and King~25. Color magnitude diagrams of the…

天体物理学 · 物理学 2009-11-13 Giovanni Carraro , Kenneth A. Janes , Jason D. Eastman

The heavily obscured open cluster Berkeley~51 shows characteristics typical of young massive clusters, even though the few previous studies have suggested older ages. We combine optical ($UBV$) and 2MASS photometry of the cluster field with…

太阳与恒星天体物理 · 物理学 2018-03-22 Ignacio Negueruela , Maria Monguió , Amparo Marco , Hugo M. Tabernero , Carlos González-Fernández , Ricardo Dorda

We have obtained medium-low resolution spectroscopy and BVI CCD imaging of Berkeley 32, an old open cluster which lies in the anticentre direction. From the radial velocities of 48 stars in the cluster direction we found that 31 of them, in…

天体物理学 · 物理学 2009-11-11 V. D'Orazi , A. Bragaglia , M. Tosi , L. Di Fabrizio , E. V. Held

We investigate two neighboring clusters in the Cygnus complex, Berkeley 86 and Berkeley 87, with a primary emphasis on the evaluation of extinction in the field of view towards and across the clusters. We also analyze their kinematic…

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…

天体物理学 · 物理学 2009-11-10 L. Di Fabrizio , A. Bragaglia , M. Tosi , G. Marconi

We observed the Galactic open cluster Berkeley 50 in order to determine its stellar content, distance, and age. We obtained UBV photometry of 1145 stars in a 12.3' $\times$ 12.3' field, and used Gaia proper motions and parallaxes to…

太阳与恒星天体物理 · 物理学 2024-04-17 Meghan Speckert , Philip Massey , Brian A. Skiff

In this study, the structural and basic astrophysical parameters of the poorly studied open cluster Berkeley 6 are calculated. Analyses of the cluster are carried out using the third photometric, spectroscopic, and astrometric data release…

星系天体物理 · 物理学 2023-06-28 S. Koc , T. Yontan

The stellar populations in the outer Galactic disk are nowadays a subject of wide interest. To contribute to a better picture of this part of the Galaxy, we have studied the nature of five marginally investigated star clusters (Collinder…

天体物理学 · 物理学 2015-06-24 Giovanni Carraro , Edgardo Costa

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…

天体物理学 · 物理学 2009-11-13 G. Carraro , G. Baume , R. Vazquez , A. Moitinho , D. Geisler

The CCD UBV(RI)KC photometry of the poorly studied open clusters Juchert 9 (Juc 9) and Berkeley 97 (Be 97), which are observed with the 0.84 m telescope at the San Pedro M\'artir National Observatory, M\'exico has been analysed. For the…

星系天体物理 · 物理学 2019-12-02 İnci Akkaya Oralhan , Raúl Michel , Yonca Karslı , Hikmet Çakmak , Hwankyung Sung , Yüksel Karataş

As part of a wider investigation of evolved massive stars in Galactic open clusters, we have spectroscopically identified three candidate classical Cepheids in the little-studied clusters Berkeley 51, Berkeley 55 and NGC 6603. Using new…

太阳与恒星天体物理 · 物理学 2018-05-23 M. E. Lohr , I. Negueruela , H. M. Tabernero , J. S. Clark , F. Lewis , P. Roche
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