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Related papers: Variable stars in the Globular Cluster NGC 2808

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We present the analysis of 11 nights of V and I time-series observations of the globular cluster NGC 1904 (M 79). Using this we searched for variable stars in this cluster and attempted to refine the periods of known variables, making use…

Solar and Stellar Astrophysics · Physics 2015-06-11 N. Kains , D. M. Bramich , R. Figuera Jaimes , A. Arellano Ferro , S. Giridhar , K. Kuppuswamy

We present new time-series CCD photometry, in the B and V bands, for the moderately metal-rich ([Fe/H] ~ -1.3) Galactic globular cluster (GC) M62 (NGC 6266). The present dataset is the largest obtained so far for this cluster, and consists…

Solar and Stellar Astrophysics · Physics 2015-05-20 R. Contreras , M. Catelan , H. A. Smith , B. J. Pritzl , J. Borissova , C. A. Kuehn

(Abridged) We present CCD BVI photometry of 85 variable stars from the field of the globular cluster NGC 6934. The photometry was obtained with the image subtraction package ISIS. 35 variables are new identifications: 24 RRab stars, 5 RRc…

Astrophysics · Physics 2009-10-31 J. Kaluzny , A. Olech , K. Z. Stanek

We analyzed the incidence and properties of RR Lyrae stars that show evidence for amplitude and phase modulation (the so-called Blazhko Effect) in a sample of $\sim$3,000 stars with LINEAR and ZTF light curve data collected during the…

Solar and Stellar Astrophysics · Physics 2025-04-09 Ema Donev , Željko Ivezić

RR Lyrae stars are classical pulsating stars. They pulsate mostly in the radial fundamental mode (RRab stars), in the radial first overtone mode (RRc stars), or in both modes simultaneously (RRd stars). Collection of variable stars from the…

Solar and Stellar Astrophysics · Physics 2016-03-18 H. Netzel , R. Smolec

Extended BV(RI)c CCD observations of SS Cnc, a short period RRab star are presented. Nearly 1400 data points in each band have been obtained spanning over 79 days during the spring of 2005. The star exhibits light curve modulation, the so…

Astrophysics · Physics 2008-11-26 J. Jurcsik , B. Szeidl , Á. Sódor , I. Dékány , Zs. Hurta , K. Posztobányi , K. Vida , M. Váradi , A. Szing

We present a ground-based time-series photometric study of stellar variability in four intermediate- to old-age open clusters NGC 2192, NGC 2266, NGC 2509, and IC 1369 based on high-cadence Cousins R-band observations obtained with the 0.6…

Solar and Stellar Astrophysics · Physics 2026-03-17 K. Belwal , D. Bisht , Ing-Guey Jiang , Mohit Singh Bisht , A. Raj , S. K. Chakrabarti , D. Bhowmick

We report here CCD $I$-band time-series photometry of a young (2$-$5 Myr) cluster NGC 2282 to identify and understand the variability of pre-main-sequence (PMS) stars. The $I$-band photometry, down to $\sim$ 20.5 mag, enables us to probe…

Astrophysics of Galaxies · Physics 2018-04-04 Somnath Dutta , Soumen Mondal , Santosh Joshi , Jessy Jose , Ramkrishna Das , Supriyo Ghosh

We present the analysis of Blazhko-type modulation in double-mode RR Lyrae (RRd) stars found in the OGLE photometry of the Galactic bulge. Modulation is detected in 15 stars. Most of them have non-typical period ratio of the radial modes.…

We report on the discovery of eleven multimode SX Phoenicis--type blue stragglers in the field of the southern globular cluster NGC 3201. In these variables both radial and non-radial modes are excited. For three variables the derived…

Astrophysics · Physics 2009-11-07 B. Mazur , W. Krzeminski , I. B. Thompson

We present V and B-band CCD photometry of 35 RR Lyr stars in the southern hemisphere globular cluster NGC 6362. Fourier decomposition of the light curves was used to estimate the basic properties of these variables. From the analysis of the…

Astrophysics · Physics 2009-10-31 A. Olech , J. Kaluzny , I. B. Thompson , W. Pych , W. Krzeminski , A. Schwarzenberg-Czerny

We report the discovery of two new variable stars in the metal-poor globular cluster NGC 288, found by means of time-series CCD photometry. We classified the new variables as SX Phoenicis due to their characteristic fundamental mode periods…

Solar and Stellar Astrophysics · Physics 2015-03-18 E. Martinazzi , S. O. Kepler , J. E. S. Costa , A. Pieres , C. Bonatto , E. Bica , L. Fraga

We report the discovery of a new subclass of double-mode RR Lyrae stars in the Large and Small Magellanic Clouds. The sample of 22 pulsating stars have been extracted from the latest edition of the OGLE collection of RR Lyrae variables in…

We present $V,I$ light curves for 12 variable stars identified in the newly discovered satellite of the Milky Way in the Bootes constellation (Belokurov et al. 2006).Our sample includes 11 RR Lyrae stars (5 first overtone, 5 fundamental…

We present a multiband (UBVRI) time-series photometric study of RR Lyrae (RRL) stars in the globular cluster Messier 53 (NGC 5024) to refine their pulsation properties and determine a precise cluster distance. The archival photometric data…

Solar and Stellar Astrophysics · Physics 2026-01-08 Shantanu A. Gaur , Nitesh Kumar , Anupam Bhardwaj , Aasheesh Raturi

We present period change rates (dP/dt) for 42 RR Lyrae variables in the globular cluster IC$\,$4499. Despite clear evidence of these period increases or decreases, the observed period change rates are an order of magnitude larger than…

We study the variable star content of the globular cluster M53 to compute the physical parameters of the constituting stars and the distance of the cluster. Covering two adjacent seasons in 2007 and 2008, new photometric data are gathered…

Solar and Stellar Astrophysics · Physics 2015-05-14 Istvan Dekany , Geza Kovacs

Time-series CCD photometric observations of the intermediate-age open cluster NGC 2099 were performed to search for variable stars. We also carried out BV photometry to study physical properties of variables in the cluster. Using V-band…

Astrophysics · Physics 2009-11-13 Y. B. Kang , S. -L. Kim , S. -C. Rey , C. -U. Lee , Y. H. Kim , J. -R. Koo , Y. -B. Jeon

We have performed a detailed study of the pulsational and evolutionary characteristics of 133 RR Lyrae stars in the globular cluster NGC5272 (M3) using highly accurate BVI data taken on 5 separate epochs. M3 seems to contain no less than…

Astrophysics · Physics 2009-11-10 C. Cacciari , T. M. Corwin , B. W. Carney