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相关论文: Variable Stars in Metal-Rich Globular Clusters. II…

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We present time-series VI photometry of the metal-rich ([Fe/H] = -0.53) globular cluster NGC 6441. Our color-magnitude diagram shows that the extended blue horizontal branch seen in Hubble Space Telescope data exists in the outermost…

天体物理学 · 物理学 2009-10-30 A. C. Layden , L. A. Ritter , D. L. Welch , T. M. A. Webb

We have undertaken a search for variable stars in the metal-rich globular cluster NGC 6441 using time-series BV photometry. The total number of variables found near NGC 6441 has been increased to ~104, with 48 new variables being found in…

天体物理学 · 物理学 2009-11-06 Barton J. Pritzl , Horace A. Smith , Marcio Catelan , Allen V. Sweigart

We have undertaken a search for variable stars in the metal-rich globular cluster NGC 6388 using time-series BV photometry. Twenty-eight new variables were found in this survey, increasing the total number of variables found near NGC 6388…

天体物理学 · 物理学 2009-11-07 Barton J. Pritzl , Horace A. Smith , Marcio Catelan , Allen V. Sweigart

We present VI-band photometry for stars in the metal-rich globular cluster NGC 6496. Our time-series data were cadenced to search for long period variables (LPVs) over a span of nearly two years, and our variability search yielded the…

We present new time-series CCD \emph{VR} photometry of the globular cluster NGC 5634. We aim to use the known RR Lyrae stars, members of the cluster, as indicators of mean metallicity and distance. Accurate coordinates, periods and an…

太阳与恒星天体物理 · 物理学 2025-07-21 A. Arellano Ferro , R. Michel , M. A. Yepez , S. Muneer , I. Bustos Fierro , Z. Prudil

We report CCD $V$ and $I$ time-series photometry of the globular cluster NGC 6333 (M9). The technique of difference image analysis has been used, which enables photometric precision better than 0.05 mag for stars brighter than $V \sim 19.0$…

In this paper, we present the analysis of time-series observations from 2013 and 2014 of five metal rich ([Fe/H] $>$ -1) globular clusters: NGC~6388, NGC~6441, NGC~6528, NGC~6638, and NGC~6652. The data have been used to perform a census of…

NGC 6441 is a bulge globular cluster with an unusual horizontal branch morphology and a rich population of RR Lyrae (RRL) and Type II Cepheid (T2C) variables that is unexpected for its relatively high metallicity. We present near-infrared…

太阳与恒星天体物理 · 物理学 2022-12-14 A. Bhardwaj , S. M. Kanbur , M. Rejkuba , M. Marconi , M. Catelan , V. Ripepi , H. P. Singh

We present a comprehensive analysis of the variable stars projected on the field of the Galactic bulge globular cluster NGC 6522, offering valuable insights into their characteristics. Using proper motions from Gaia DR3, we aim to…

太阳与恒星天体物理 · 物理学 2023-10-26 A. Arellano Ferro , Z. Prudil , M. A. Yepez , I. Bustos Fierro , A. Luna

[Abridged] We present the results of a Hubble Space Telescope snapshot program to survey the inner region of the globular cluster NGC 6441 for its variable stars. A total of 57 variable stars was found including 38 RR Lyrae stars, 6…

New time-series VI CCD photometry of the globular cluster NGC 6362 is studied with the aim of estimating the reddening, mean metallicity and distance of the cluster from its population of RR Lyrae stars. The Fourier decomposition of…

太阳与恒星天体物理 · 物理学 2018-06-13 A. Arellano Ferro , J. A. Ahumada , I. H. Bustos Fierro , J. H. Calderón , N. I. Morrell

We present time-series $BVI$ photometry for the Galactic globular cluster NGC 6402 (M14). The data consists of $\sim$137 images per filter, obtained using the 0.9m and 1.0m SMARTS telescopes at the Cerro Tololo Inter-American Observatory.…

太阳与恒星天体物理 · 物理学 2018-02-28 C. Contreras Peña , M. Catelan , F. Grundahl , A. W. Stephens , H. A. Smith

We have calculated the physical parameters of the RR Lyrae stars in the globular cluster NGC~4147 via the Fourier decomposition of their light curves, using new data and well-established semi-empirical calibrations and zero points. The mean…

太阳与恒星天体物理 · 物理学 2018-03-15 A. Arellano Ferro , F. C. Rojas Galindo , S. Muneer , Sunetra Giridhar

We report a result of our near-infrared repeated observations of Mira variables in the globular clusters NGC 6388 and 6441. These two clusters are known as peculiar clusters with blue horizontal branch stars and RR Lyr variables which are…

天体物理学 · 物理学 2007-05-23 Noriyuki Matsunaga , the IRSF/SIRIUS team

We present the results from $VI$ CCD time-series photometry of the globular cluster M13 (NGC 6205). From the Fourier decomposition of the light curves of RRab and RRc stars we found an average metallicity of [Fe/H]zw = -1.58 $\pm$ 0.09. The…

太阳与恒星天体物理 · 物理学 2019-03-13 D. Deras , A. Arellano Ferro , C. Lázaro , I. H. Bustos Fierro , J. H. Calderón , S. Muneer , Sunetra Giridhar

NGC 6388 and NGC 6441 are anomalies among Galactic globular clusters in that they cannot be readily place into either Oosterhoff group I or Oosterhoff group II despite their significant numbers of RR Lyrae variables. The mean pulsation…

天体物理学 · 物理学 2009-10-31 Barton Pritzl , Horace A. Smith , Marcio Catelan , Allen V. Sweigart

Low resolution spectra have been used to measure individual metal abundances of RR Lyrae stars in NGC 6441, a Galactic globular cluster known to have very unusual horizontal branch morphology and periods of the RR Lyrae stars for its high…

We present a CCD $VI$ time-series analysis of the globular cluster NGC 6139 and its variable star population. Using the astrometric data available in $Gaia$-DR3 we performed a membership analysis that enabled the construction of a clean…

太阳与恒星天体物理 · 物理学 2023-06-28 M. A. Yepez , A. Arellano Ferro , I. Bustos Fierro , A. Luna

We present a study of variable stars in globular cluster NGC 6401. The cluster is only $5.3\degr$ away from the Galactic centre and suffers from strong differential reddening. The photometric precision afforded us by difference image…

太阳与恒星天体物理 · 物理学 2016-11-01 Y. Tsapras , A. Arellano Ferro , D. M. Bramich , R. Figuera Jaimes , N. Kains , R. Street , M. Hundertmark , K. Horne , M. Dominik , C. Snodgrass

A rich harvest of RR Lyrae stars has been identified for the first time in B514, a metal-poor ([Fe/H] = 1.95 +/- 0.10 dex) globular cluster of the Andromeda galaxy (M31), based on Hubble Space Telescope Wide Field Planetary Camera 2 and…

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