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相关论文: Deep, Wide-field CCD Photometry for the Open Clust…

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We present analysis of deep CCD photometry for the very rich, old open star cluster NGC 6819. These CFH12K data results represent the first of nineteen open star clusters which were imaged as a part of the CFHT Open Star Cluster Survey. We…

NGC 3532 is an extremely rich open cluster embedded in the Galactic disc, hitherto lacking a comprehensive, documented membership list. We provide membership probabilities from new radial velocity observations of solar-type and low-mass…

太阳与恒星天体物理 · 物理学 2019-02-06 D. J. Fritzewski , S. A. Barnes , D. J. James , A. M. Geller , S. Meibom , K. G. Strassmeier

Images and spectra of the open cluster NGC 3105 have been obtained with GMOS on Gemini South. The (i', g'-i') color-magnitude diagram (CMD) constructed from these data extends from the brightest cluster members to g'~23. This is 4 - 5 mag…

星系天体物理 · 物理学 2017-03-22 T. J. Davidge

We present deep CCD photometry of the very rich, intermediate aged (similar to the Hyades) open star cluster NGC 2099 (M37). The V, B-V color-magnitude diagram (CMD) for the cluster shows an extremely well populated and very tightly…

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 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…

天体物理学 · 物理学 2009-11-07 S. Ortolani , G. Carraro , S. Covino , E. Bica , B. Barbuy

We present the results of a photometric and spectroscopic study of the white dwarf candidate members of the intermediate age open clusters NGC3532 and NGC2287. Of the nine objects investigated, it is determined that six are probable members…

太阳与恒星天体物理 · 物理学 2009-11-13 P. D. Dobbie , R. Napiwotzki , M. R. Burleigh , K. Williams , R. G. Sharp , M. A. Barstow , S. L. Casewell , I. Hubeny

In a sample of six young open clusters we investigated 1753 objects using the narrow band, three filter Delta a photometric system resulting in the detection of eleven bona-fide magnetic chemically peculiar (CP) stars and five Be or…

天体物理学 · 物理学 2009-11-11 E. Paunzen , M. Netopil , I. Kh. Iliev , H. M. Maitzen , A. Claret , O. I. Pintado

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 report on a new, wide field ($20^{\prime} \times 20^{\prime}$), multicolor ($UBVI$), photometric campaign in the area of the nearby old open cluster NGC 2112. At the same time, we provide medium-resolution spectroscopy of 35 (and…

天体物理学 · 物理学 2009-11-13 Giovanni Carraro , Sandro Villanova , Pierre Demarque , Christian Moni Bidin , Ginny McSwain

We present deep BVI observations of the core of M35 and a nearby comparison field obtained at the WIYN 3.5m telescope under excellent seeing. These observations display the lower main sequence in BV and VI CMDs down to V = 23.3 and 24.6,…

天体物理学 · 物理学 2009-11-07 Ted von Hippel , Aaron Steinhauer , Ata Sarajedini , Constantine P. Deliyannis

Three new photometric CCD-based datasets are presented for NGC~6791. They consist of deep UBV photometry (to $V_{lim} =24$, $B_{lim}=24$, $U_{lim} = 23$) of the central parts of the cluster and of selected fields around it, and of…

天体物理学 · 物理学 2016-08-30 Janusz Kaluzny , Slavek Rucinski

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

Accurate and deep BVI CCD photometry is presented for the core regions of six southern compact open clusters (supplemented in one case by U and R bands). These clusters generally have only scanty photometric data published, in some case…

天体物理学 · 物理学 2009-11-10 Giovanni Carraro , Ulisse Munari

Photometry in the B and V bands is presented for the southern stellar groups NGC 1901 and NGC 1252. NGC 1901 is often described as an open cluster while NGC 1252 consists of a concentration of about 20 stars centered approx 20' north of the…

天体物理学 · 物理学 2009-11-06 D. B. Pavani , E. Bica , C. M. Dutra , H. Dottori , B. X. Santiago , G. Carranza , R. J. Diaz

We report the results of a CCD imaging survey, complimented by astrometric and spectroscopic follow-up studies, that aims to probe the fate of heavy-weight intermediate mass stars by unearthing new, faint, white dwarf members of the rich,…

太阳与恒星天体物理 · 物理学 2015-06-04 P. D. Dobbie , A. Day-Jones , K. A. Williams , S. L. Casewell , M. R. Burleigh , N. Lodieu , Q. A. Parker , R. Baxter

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.…

太阳与恒星天体物理 · 物理学 2015-10-14 B. A. Twarog , B. J. Anthony-Twarog , C. P. Deliyannis , D. T. Thomas

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 present and discuss broad band CCD $UBV(I)_C$ photometry and low resolution spectroscopy for stars in the region of the open cluster NGC 6996, located in the North America Nebula. The new data allow us to tightly constrain the basic…

天体物理学 · 物理学 2009-11-10 Sandro Villanova , Gustavo Baume , Giovanni Carraro , Anna Geminale

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
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