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Related papers: Variable Stars in Galactic Globular Clusters

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In this paper we revisit observational data concerning RR Lyrae stars in Galactic globular clusters, presenting frequency histograms of fundamentalized periods for the 32 clusters having more than 12 pulsators with well recognized period…

Astrophysics · Physics 2009-11-10 M. Castellani , F. Caputo , V. Castellani

[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…

We present a comprehensive catalog of 2824 RR Lyrae stars (RRLs) residing in 115 Galactic globular clusters (GCs). Our catalog includes 1594 fundamental-mode (RRab), 824 first-overtone (RRc), and 28 double-mode (RRd) RRLs, as well as 378…

Solar and Stellar Astrophysics · Physics 2024-02-15 Mauricio Cruz Reyes , Richard I. Anderson , Lucas Johansson , Henryka Netzel , Zoé Medaric

This is the second in a series of papers studying the variable stars in Large Magellanic Cloud globular clusters. The primary goal of this series is to study how RR Lyrae stars in Oosterhoff-intermediate systems compare to their…

Solar and Stellar Astrophysics · Physics 2015-06-11 Charles A. Kuehn , Horace A. Smith , Marcio Catelan , Barton J. Pritzl , Nathan De Lee , Jura Borissova

CCD observations for 10 (6 previously known and 4 newly discovered) of the 11 RR Lyrae variables in NGC 5897 have been analysed. The period-luminosity and period-amplitude plots indicate that the population of RR Lyrae variables in NGC 5897…

Astrophysics · Physics 2009-11-06 Christine M. Clement , Jason F. Rowe

We obtained a series of more than two hundred R-band CCD images for the crowded central (115"x77") region of the metal-poor globular cluster M15 with an angular resolution of 0.5"-0.9" in most images. Optimal image subtraction was used to…

Astrophysics · Physics 2009-11-10 Alexander P. Zheleznyak , Valery V. Kravtsov

We present a new, deep (V ~ 26) study of the Galactic globular cluster NGC 2419 based on B,V,I time-series CCD photometry over about 10 years and extending beyond the cluster published tidal radius. We have identified 101 variable stars of…

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…

We present a new search for variable stars in the Galactic globular cluster M28 (NGC 6626). The search is based on a series of BVI images obtained with the SMARTS Consortium's 1.3m telescope at Cerro Tololo Inter-American Observatory,…

Solar and Stellar Astrophysics · Physics 2015-06-05 G. Prieto , M. Catelan , R. Contreras Ramos , B. J. Pritzl , H. A. Smith , J. Alonso-Garcia

We present a long-term project aimed at completing the census of (bright) variable stars in Galactic globular clusters. While our main aim is to obtain a reliable assessment of the populations of RR Lyrae and type II Cepheid stars in the…

We report on the discovery of a large number of RR Lyrae variable stars in the moderately metal-rich Galactic globular cluster M62 (NGC 6266), which places it among the top three most RR Lyrae-rich globular clusters known. Likely members of…

Astrophysics · Physics 2009-11-10 R. Contreras , M. Catelan , H. A. Smith , B. J. Pritzl , J. Borissova

Using an image subtraction method we have searched for variable stars in the globular cluster M14. We confirmed 62 previously known catalogued variables. In addition to the previoulsy known variables we have identified 71 new variables. We…

Solar and Stellar Astrophysics · Physics 2012-05-15 Kyle E. Conroy , Andrew N. Darragh , Zheyu J. Liu , Brian W. Murphy

Globular clusters are both primary fossils of galactic evolution and formation and are ideal laboratories for constraining the evolution of low-mass and metal-poor stars. RR Lyrae and type II Cepheid variables are low-mass, radially…

Solar and Stellar Astrophysics · Physics 2022-02-16 Anupam Bhardwaj

We present the results of a search for variable stars in the globular cluster NGC 5286, which has recently been suggested to be associated with the Canis Major dwarf spheroidal galaxy. 57 variable stars were detected, only 19 of which had…

We present a new study of the variable star population in globular cluster 5 of the Fornax dwarf spheroidal galaxy, based on B and V time series photometry obtained with the MagIC camera of the 6.5 m Magellan Clay telescope and…

The first calibrated broadband BVI time-series photometry is presented for the variable stars in NGC 2808, with observations spanning a range of twenty-eight years. We have also redetermined the variability types and periods for the…

Solar and Stellar Astrophysics · Physics 2015-06-12 Andrea Kunder , Peter B. Stetson , Marcio Catelan , Alistair R. Walker , Pia Amigo

We present a search for variable stars in the Fornax dwarf galaxy covering an area of 1/2 a square degree. We have ~30 epochs of VI data. We found and determined periods for more than 500 RR Lyrae, 17 anomalous Cepheids, 6 Population II…

Astrophysics · Physics 2009-11-07 D. Bersier , P. R. Wood

Results of a search for variable stars in the central region of the globular cluster M13 are presented. Prior to this study, 36 variable and suspected variable stars were known in this cluster (Osborn 2000; Clement et al. 2001). Of these…

Astrophysics · Physics 2009-11-07 G. Kopacki , Z. Kolaczkowski , A. Pigulski

We present the results of our new study of known RR Lyrae variable stars. All observations available for these stars in the Catalina Surveys were analyzed, and double-mode variations were identified. We studied the Petersen diagram and…

Solar and Stellar Astrophysics · Physics 2018-03-14 A. V. Khruslov

We describe here results of a photometric time-sequence survey of the globular cluster M3 (NGC 5272), in a search for contact and detached eclipsing binary stars. We have discovered only one likely eclipsing binary and one SX Phe type star…

Astrophysics · Physics 2016-08-30 J. Kaluzny , R. W. Hilditch , C. Clement , S. M. Rucinski
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