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Related papers: Are all RR Lyrae stars modulated?

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

Solar and Stellar Astrophysics · Physics 2015-05-28 Charles A. Kuehn , Horace A. Smith , Márcio Catelan , Barton J. Pritzl , Nathan De Lee , Jura Borissova

We present the catalog of RR Lyrae stars from 2.4 square degrees of central parts of the Small Magellanic Cloud (SMC). The photometric data were collected during four years of the OGLE-II microlensing survey. Photometry of each star was…

We present a careful and detailed light curve analysis of RR Lyrae stars in the Small Magellanic Cloud (SMC) discovered by the Optical Gravitational Lensing Experiment (OGLE) project. Out of 536 single mode RR Lyrae stars selected from the…

Solar and Stellar Astrophysics · Physics 2015-05-14 Sukanta Deb , Harinder P. Singh

The analysis of the multicolour photometric observations of MW Lyr, a large modulation amplitude Blazhko variable, shows for the first time how the mean global physical parameters vary during the Blazhko cycle. About 1-2 percent changes in…

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

A CCD VI imaging time-series over 11-year is employed to explore the light curves of stars in the field of Palomar 2. We discovered 20 RRab and 1 RRc variables. A revision of Gaia-DR3 data enabled us to identify 10 more variables and…

Solar and Stellar Astrophysics · Physics 2023-04-12 A. Arellano Ferro , I. Bustos Fierro , S. Muneer , S. Giridhar

The knowledge of accurate stellar parameters is a keystone in several fields of stellar astrophysics, such as asteroseismology and stellar evolution. Although the fundamental parameters can be derived both from spectroscopy and multicolour…

Solar and Stellar Astrophysics · Physics 2015-05-18 Katrien Kolenberg , Luca Fossati , Denis Shulyak , Holger Pikall , Thomas G. Barnes , Oleg Kochukhov , Vadim Tsymbal

Recent theoretical and observational findings breathed new life into the field of RR Lyrae stars. The ever more precise and complete measurements of the space asteroseismology missions revealed new details, such as the period doubling and…

Solar and Stellar Astrophysics · Physics 2015-06-11 L. Molnár , Z. Kolláth , R. Szabó , E. Plachy

The lack of RR Lyr stars in binary systems is an atypical fact when we compared it to other classes of variables. Therefore, it has become a challenge for observers to detect an RR Lyr variable in a binary system. The RR Lyr variable KIC…

We discuss the results of a systematic search for multiperiodic pulsations in Galactic Bulge Delta Scuti and RR Lyrae stars. Six "normal" double-mode variables pulsating in two radial modes have been identified (5 Delta Scuti-type and 1 RR…

Astrophysics · Physics 2007-05-23 P. Moskalik , E. Poretti

We present V-band CCD photometry of 65 RR Lyr variables from the globular cluster M5. We have estimated the basic physical parameters for 16 RRc stars and 26 RRab stars using a Fourier decomposition of the light curves of the variables. The…

Astrophysics · Physics 2007-05-23 J. Kaluzny , A. Olech , I. Thompson , W. Pych , W. Krzeminski , A. Schwarzenberg-Czerny

We present the analysis of the CoRoT star 105288363, a new Blazhko RR Lyrae star of type RRab (f0 = 1.7623 c/d), observed with the CoRoT space craft during the second long run in direction of the galactic center (LRc02, time base 145 d).…

Solar and Stellar Astrophysics · Physics 2016-08-14 E. Guggenberger , K. Kolenberg , E. Chapellier , E. Poretti , R. Szabó , J. M. Benkő , M. Paparó

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

RR Lyrae stars are of great importance for investigations of Galactic structure. However, a complete compendium of all RR-Lyraes in the solar neighbourhood with accurate classifications and coordinates does not exist to this day. Here we…

Astrophysics · Physics 2009-11-11 Gisela Maintz

Context. A number of RR Lyrae stars show variable mean magnitudes in the OGLE survey light curves of the Galactic bulge. Hitherto this phenomenon was not studied, as it was generally assumed to be related to problems with the photometry.…

Double-mode RR Lyr type stars are important for studies of properties of horizontal-branch stars. In particular, two periods coupled with spectral properties give a mass estimate that is independent of evolutionary models. Here, we present…

Solar and Stellar Astrophysics · Physics 2014-07-07 R. Poleski

We report the results of our study of lightcurve modulation in a sample of 493 RR1 variables from the OGLE-III survey of galactic bulge fields. Each object in this list has 1500 or more I-band observations. We compare our findings with…

Solar and Stellar Astrophysics · Physics 2013-10-03 Douglas L. Welch , Grant Foster

We present measurements of the periods, amplitudes, and types of 74 RR Lyrae stars in the globular cluster M15 derived from Nickel 1 m telescope observations conducted at LickObservatory in 2019 and 2020. Of these RR Lyrae stars, two were…

Solar and Stellar Astrophysics · Physics 2021-01-13 Andrew M. Hoffman , Yukei S. Murakami , WeiKang Zheng , Benjamin E. Stahl , Alexei V. Filippenko

We report the discovery of an RR Lyrae star that experienced a switching of its pulsation mode. OGLE-BLG-RRLYR-12245 was discovered as a double-mode RRd star from the observations conducted in years 2001-2006 during the third phase of the…

We present a comprehensive photometric study of RR Lyrae stars in the M3 globular cluster, utilising a vast dataset of 3140 optical ($UBVRI$) CCD images spanning 35 years from astronomical data archives. We have successfully identified…

Solar and Stellar Astrophysics · Physics 2024-05-28 Nitesh Kumar , Anupam Bhardwaj , Harinder P. Singh , Marina Rejkuba , Marcella Marconi , Philippe Prugniel