English
Related papers

Related papers: The intermediate-age open cluster NGC 2112

200 papers

Multi-wavelength CCD photometry over 21 years has been used to produce deep color-magnitude diagrams together with light curves for the variables in the Galactic globular cluster NGC 5824. Twenty-one new cluster RR Lyrae stars are…

The first CCD photometric investigation of the open cluster NGC 7296 up to now was performed within the narrow band Delta a photometric system, which enables us to detect peculiar objects. A deeper investigation of that cluster followed,…

Astrophysics · Physics 2009-11-11 M. Netopil , E. Paunzen , H. M. Maitzen , A. Claret , K. Pavlovski , E. Tamajo

We report on deep (V $\approx$ 24.0) $VI$ CCD photometry of 3 fields centered in the regions of the old open clusters Saurer A, B and C. In the case of Saurer A, which is considered one of the oldest known open cluster, we also provide a…

Astrophysics · Physics 2009-11-10 Giovanni Carraro , Gustavo Baume

We present new isochrone fits to colour-magnitude diagrams of the Galactic globular clusters NGC\,288, NGC\,362, and NGC\,6218 (M12). We utilize a lot of photometric bands from the ultraviolet to mid-infrared by use of data from the {\it…

We present CCD photometric and mass function study of 9 young Large Magellanic Cloud star clusters namely NGC 1767, NGC 1994, NGC 2002, NGC 2003, NGC 2006, SL 538, NGC 2011, NGC 2098 and NGC 2136. The BVRI data reaching down to V ~ 21 mag,…

Astrophysics · Physics 2009-11-13 B. Kumar , R. Sagar , J. Melnick

We report the results of a time-series CCD photometric survey of variable stars in the field of the open cluster NGC 2126. In about one square degree field covering the cluster, a total number of 21 variable candidates are detected during…

Solar and Stellar Astrophysics · Physics 2009-07-22 Shun-Fang Liu , Zhen-Yu Wu , Xiao-Bin Zhang , Jiang-Hua Wu , Jun Ma , Zhao-Ji Jiang , Jian-Sheng Chen , Xu Zhou

We present multi-colour broad band CCD photometric observations of a few thousands of stars located region of the galactic globular clusters NGC 1904 and NGC 6341. These observations are used to generate their deep colour magnitude diagrams…

Astrophysics · Physics 2007-05-23 Alok C. Gupta

From uvby photometry of 75 stars in the direction of NGC 7063 we were able to determine membership of some stars and fix the distance (722 +- 105 pc), log age (of 8.146) and reddening (E(b-y) = 0.091 +- 0.039 mag) for the cluster.

Astrophysics · Physics 2007-07-17 J. H. Pena , L. Fox Machado , R. Garrido

We present deep wide-field optical CCD photometry and mid-infrared Spitzer/IRAC and MIPS 24micron data for about 100,000 stars in the young open cluster IC 1805. The members of IC 1805 were selected from their location in the various…

Solar and Stellar Astrophysics · Physics 2020-12-09 Hwankyung Sung , Michael S. Bessell , Moo-Young Chun , Jonghyuk Yi , Y. Naze , Beomdu Lim , R. Karimov , G. Rauw , Byeong-Gon Park , Hyeonoh Hur

We present WFPC2 and ground-based VI photometry of NGC 121 and a nearby field in the outer SMC. For NGC 121, we measure a true distance modulus of (m-M)0 = 18.96 +/- 0.04 (distance of 61.9 +/- 1.1 kpc), age of 10.6 +/- 0.5 Gyr, metallicity…

We present VI photometry of the metal-poor inner halo globular clusters NGC6293 and NGC6541 using the planetary camera of the WFPC2 on board HST. Our color-magnitude diagrams of the clusters show well-defined BHB populations, consistent…

Astrophysics · Physics 2008-11-26 Jae-Woo Lee , Bruce W. Carney

The results of astrometric and photometric investigations of the poorly studied open cluster NGC 1513 are presented. The proper motions of 353 stars with the root-mean-square error of 1.9 mas/yr were obtained by means of the automated…

To progress in galactic studies based on open clusters, e.g. cluster formation rate or kinematical properties, one needs to improve the number of open clusters observed. However, only half of the 1700 known galactic open clusters have been…

Astrophysics · Physics 2009-11-11 M. Netopil , H. M. Maitzen , E. Paunzen , A. Claret

Precision uvbyCaHbeta photometry of the nearby old open cluster, NGC 752, is presented. The mosaic of CCD fields covers an area ~42' on a side with internal precision at the 0.005 to 0.010 mag level for the majority of stars down to V~15.…

Solar and Stellar Astrophysics · Physics 2015-10-14 B. A. Twarog , B. J. Anthony-Twarog , C. P. Deliyannis , D. T. Thomas

The results of medium-band photometry of 1037 stars in the area of old open cluster NGC 7142 down to V = 20.1 mag in the Vilnius seven-colour system are presented. Photometric results are used to classify in spectral and luminosity classes…

Astrophysics of Galaxies · Physics 2013-12-05 V. Straizys , M. Maskoliunas , R. P. Boyle , K. Zdanavicius , J. Zdanavicius , V. Laugalys , A. Kazlauskas

We present results of the first extensive and deep CCD photometric survey carried out in the field of the open cluster Trumpler 27, an object in the constellation of Sagittarius not far from the Galaxy center. We look for young stars clumps…

Astrophysics of Galaxies · Physics 2015-06-03 Gabriel Perren , Rubén Vázquez , Giovanni Carraro

We present a photometric and spectroscopic study of the young open cluster NGC 7419, which is know to host a large number of classical Be stars for reasons not well understood. Based on CCD photometric observations of 327 stars in UBV…

Astrophysics · Physics 2009-11-11 Annapurni Subramaniam , Blesson Mathew , Bhuwan Chandra Bhatt , S. Ramya

We present BV photometry of the Galactic globular cluster NGC 5286, based on 128 V frames and 133 B frames, and covering the entire face of the cluster. Our photometry reaches almost two magnitudes below the turn-off level, and is…

We present new astrophysical parameters for the open cluster NGC~6793 based on new CCD $UBV(RI)_{KC}$ photometry. We derived a reddening of $E(B-V) = 0.24 \pm 0.02$~mag and a heavy element abundance of $Z = 0.024$ ($[Fe/H] = +0.20$~dex).…

Recently, a noticeable number of new star clusters was identified in the outskirts of the Large Magellanic Cloud (LMC) populating the so-called star cluster age gap, a space of time (~ 4-12 Gyr) where the only known star cluster is…

Astrophysics of Galaxies · Physics 2021-03-31 Andrés E. Piatti