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To study the crucial range of Galactocentric distances between 12 and 16 kpc, where little information is available, we have obtained VI CCD imaging of Berkeley 20 and BVI CCD imaging of Berkeley 66 and Tombaugh 2, three distant, old open…

星系天体物理 · 物理学 2015-05-20 Gloria Andreuzzi , Angela Bragaglia , Monica Tosi , Gianni Marconi

We report the first results from deep ACS imaging of ten classical globular clusters in the far outer regions (15 < R_p < 100 kpc) of M31. Eight of the clusters, including two of the most remote M31 globular clusters presently known, are…

天体物理学 · 物理学 2009-11-11 A. D. Mackey , A. Huxor , A. M. N. Ferguson , N. R. Tanvir , M. Irwin , R. Ibata , T. Bridges , R. A. Johnson , G. Lewis

We present photometry in the J and K near-infrared bands for two regions centered on the young open clusters NGC 1893 and Berkeley 86. We study 700 stars down to K = 17 in the field of NGC 1893, and about 2000 stars in the field of Berkeley…

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

We present deep JHK photometry of the old and metal-rich open cluster NGC 6791. The photometry reaches below the main sequence turn-off to K = 16.5 mag. We combine our photometry with that from Stetson, Bruntt, & Grundahl (2003) to provide…

天体物理学 · 物理学 2014-10-13 Bruce W. Carney , Jae-Woo Lee , Benjamin Dodson

Color Magnitude Diagrams (CMDs) of individual stars in 8 Globular Clusters in M31 down to about 1 mag fainter (V$\sim 26.5$) than the Horizontal Branch have been obtained with the Hubble Space Telescope. In particular, we observed G280 and…

Deep and extensive CCD photometric observations $UBV(RI)_{C}H_{\alpha}$ were carried out in the area of the open cluster NGC 3293. The new data set allows to see the entire cluster sequence down to $M_{V} \approx +4.5$, revealing that stars…

天体物理学 · 物理学 2011-05-23 Gustavo Baume , Ruben Vazquez , Giovanni Carraro , Alejandro Feinstein

CCD photometry on the intermediate-band vbyCaHbeta system is presented for the metal-rich, old open cluster, NGC 6791. Preliminary analysis led to [Fe/H] above +0.4 with an anomalously high reddening and an age below 5 Gyr. A revised…

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

We present multi-colour time-series CCD photometry of the solar-age galactic open cluster M67 (NGC 2682). About 3600 frames spread over 28 nights were obtained with the 1.5 m Russian-Turkish and 1.2 m Mercator telescopes. High-precision…

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 have used deep ACS/WFC images of M33 to check nature of extended objects detected by the ground based survey of Zloczewski et al. (2008). A total of 24 candidates turned out to be genuine compact stellar clusters. In addition we detected…

太阳与恒星天体物理 · 物理学 2009-03-24 K. Zloczewski , J. Kaluzny

We present new multiband photometry for the Galactic globular cluster IC 4499 extending well past the main sequence turn-off in the U, B, V, R, I, and DDO51 bands. This photometry is used to determine that IC4499 has an age of 12 pm 1 Gyr…

M71 is a nearby, metal-rich globular cluster at low Galactic latitude, where field contamination and spatially variable extinction complicate colour-magnitude diagrams (CMDs) and the identification of cluster member variable stars. Our aims…

星系天体物理 · 物理学 2026-05-13 C. C. Cortés , D. Deras , A. Arellano Ferro , S. Muneer , I. H. Bustos Fierro

The Galactic globular cluster system is incomplete, especially in the low latitude regions of the Galactic bulge and disk. We report the physical characterization of twelve star clusters in the Milky Way, most of which are explored here for…

We present broad-band (U, V, I,and H) and narrow-band(H-alpha+[N II] and Paschen-alpha) images of the circumnuclear starburst rings in two nearby spiral galaxies, NGC 1512 and NGC 5248, obtained with WFPC2 and NICMOS on HST. Combined with…

天体物理学 · 物理学 2009-11-06 Dan Maoz , Aaron J. Barth , Luis C. Ho , Amiel Sternberg , Alexei V. Filippenko

We investigate the nature of 4 young and low-mass open clusters (OCs) located in the $2^{nd}$ and $3^{rd}$ quadrants with near-IR 2MASS photometry (errors $<0.1$ mag). After field decontamination, the colour-magnitude diagrams (CMDs)…

星系天体物理 · 物理学 2015-05-13 Charles Bonatto , Eduardo Bica

We present stellar photometry in the UBV passbands for the globular cluster M5 = NGC5904. The observations, short-exposured photographic plates and CCD frames, were obtained in the RC-focus of the 2m telescope of the Natl. Astron. Obs.…

天体物理学 · 物理学 2009-11-06 Haralambi Markov , Nedka Spassova , Plamen Baev

We present UBV CCD photometry and low-resolution spectra of stars in the field of the young open cluster NGC 146. UBV photometry of 434 stars were used to estimate the E(B$-$V) reddening of 0.55 $\pm$ 0.04 mag and BV photometry of 976 stars…

天体物理学 · 物理学 2009-11-11 A. Subramaniam , D. K. Sahu , R. Sagar , P. Vijitha , ;

New photoelectric seven-color observations in the Vilnius system are presented for 65 stars in the region of the open cluster NGC 752. Based on individual stars with accurate photometric classifications, we determine the apparent distance…

天体物理学 · 物理学 2008-11-26 S. Bartasiute , V. Deveikis , V. Straizys , A. Bogdanovicius

NGC 6819 is a richly populated, older open cluster situated within the Kepler field. A CCD survey of the cluster on the uvbyCaHbeta system, coupled with proper-motion membership, has been used to isolate 382 highly probable, single-star…

太阳与恒星天体物理 · 物理学 2015-06-22 B. J. Anthony-Twarog , C. P. Deliyannis , B. A. Twarog

The post-starburst region B in M82 and its massive star cluster component have been the focus of multiple studies, with reports that there is a large population of coeval clusters of age ~1 Gyr, which were created with a Gaussian initial…

天体物理学 · 物理学 2009-12-04 I. S. Konstantopoulos , N. Bastian , L. J. Smith , G. Trancho , M. S. Westmoquette , J. S. Gallagher