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Related papers: A Study of RR1 Lightcurve Modulation in OGLE_III B…

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We briefly discuss three cases of RR~Lyrae variable stars with Blazhko modulation from the OGLE Galactic bulge collection. In one of the discussed stars modulation with two periods is detected, in other star, we detect three Blazhko…

Solar and Stellar Astrophysics · Physics 2016-01-12 Karolina Bakowska , Radoslaw Smolec

The number of stars observed by the Optical Gravitational Lensing Experiment (OGLE) project in the Galactic bulge offers an invaluable chance to study RR Lyrae stars in a statistical manner. We used data of 3141 fundamental-mode RR Lyrae…

Solar and Stellar Astrophysics · Physics 2020-03-10 M. Skarka , Z. Prudil , J. Jurcsik

We present the analysis of the Blazhko effect - quasi-periodic modulation of pulsation amplitude and/or phase - in the Galactic bulge first overtone RR Lyrae stars (RRc). We used the data gathered during the fourth phase of the Optical…

Solar and Stellar Astrophysics · Physics 2018-12-14 Henryka Netzel , Radoslaw Smolec , Igor Soszynski , Andrzej Udalski

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 present the first paper of a series focused on the Blazhko effect in RR Lyrae type stars pulsating in the fundamental mode, that are located in the Galactic bulge. A~comprehensive overview about the incidence rate and light-curve…

Solar and Stellar Astrophysics · Physics 2017-01-25 Zdenek Prudil , Marek Skarka

We present the results of a systematic search for multiperiodic pulsators among the Galactic Bulge RR Lyrae stars of the OGLE-1 sample. We identify one "canonical" double-mode variable (RRd star) pulsating in two radial modes. In 38 stars…

Astrophysics · Physics 2009-11-07 P. Moskalik , E. Poretti

We present our results of searching for differences in light curves of modulated and non-modulated RRab stars in the Galactic bulge. We examined a sample of more than 8000 stars. The most important results are that Blazhko stars have…

Solar and Stellar Astrophysics · Physics 2018-09-12 M. Skarka , Z. Prudil

The period-change behaviour of 134 RR Lyrae stars in the globular cluster Messier 3 (M3) is investigated on the ~120-year time base of the photometric observations. The mean period-change rates (\beta \approx 0.01 d Myr^-1) of the…

Solar and Stellar Astrophysics · Physics 2015-05-30 J. Jurcsik , G. Hajdu , B. Szeidl , K. Oláh , J. Kelemen , Á. Sódor , A. Saha , P. Mallick , J. Claver

The eleventh part of the OGLE-III Catalog of Variable Stars (OIII-CVS) contains 16836 RR Lyr stars detected in the OGLE fields toward the Galactic bulge. The total sample is composed of 11756 RR Lyr stars pulsating in the fundamental mode…

We present the most comprehensive picture ever obtained of the central parts of the Milky Way probed with RR Lyrae variable stars. This is a collection of 38257 RR Lyr stars detected over 182 square degrees monitored photometrically by the…

Blazhko stars from the extended $BVI_{\mathrm C}$ time series of RRab stars in the globular cluster, M3, are analysed. This is the largest sample of Blazhko stars with full details of their Blazhko properties in a homogeneous stellar…

Solar and Stellar Astrophysics · Physics 2019-10-09 Johanna Jurcsik

The ground-based Konkoly Blazhko Survey I and II aim to collect accurate, extended, multicolour light curves of galactic field RRab stars in order to determine the incidence rate of the modulation in the sample, to study the modulation in…

Solar and Stellar Astrophysics · Physics 2011-01-27 Ádám Sódor

Extended CCD monitoring of RR Gem revealed that it is a Blazhko type RRab star with the shortest Blazhko period (7.23d) and smallest modulation amplitude (Delta Mmax<0.1 mag) currently known. The short period of the modulation cycle enabled…

The light curves of 50 RRab (RR0) stars in M5 collected in Paper I are investigated to detect Blazhko modulation. 18 Blazhko stars are identified, and modulation is suspected in two additional cases. The mean pulsation period of Blazhko…

Solar and Stellar Astrophysics · Physics 2015-05-20 J. Jurcsik , B. Szeidl , C. Clement , Zs. Hurta , M. Lovas

A new, extended time-series photometry of M3 RR Lyrae stars has revealed that four of the ten double-mode stars show large-amplitude Blazhko modulation of both radial modes. The first, detailed analysis of the peculiar behavior of the…

Solar and Stellar Astrophysics · Physics 2015-06-23 J. Jurcsik , P. Smitola , G. Hajdu , J. Nuspl

We present a complete set of OGLE photometric measurements for 214 RR Lyrae variables in the Galactic bulge, based on four observing seasons: 1992-95. These are mostly I-band measurements, with some V-band observations obtained mainly in…

Astrophysics · Physics 2009-09-25 Arkadiusz Olech

The analysis of recent, extended multicolour CCD and archive photoelectric, photographic and visual observations has revealed several important properties of RZ Lyr, an RRab-type variable exhibiting large-amplitude Blazhko modulation. On…

We present a catalog of 1888 fundamental-mode RR Lyrae stars detected in the Galactic bulge fields of the second phase of the Optical Gravitational Lensing Experiment (OGLE). The catalog includes basic parameters of the light curves,…

Astrophysics · Physics 2008-11-26 Matthew J. Collinge , Takahiro Sumi , Daniel Fabrycky

We present first direct evidence of modulation in the $K$-band of Blazhko-type RR Lyrae stars that are identified by their secular modulations in the I-band data of OGLE-IV. A method has been developed to decompose the $K$-band light…

Solar and Stellar Astrophysics · Physics 2018-01-31 J. Jurcsik , G. Hajdu , I. Dékány , J. Nuspl , M. Catelan , E. K. Grebel

A systematic survey to establish the true incidence rate of the Blazhko modulation among short-period, fundamental-mode, Galactic field RR Lyrae stars has been accomplished. The Konkoly Blazhko Survey (KBS) was initiated in 2004. Since then…

Solar and Stellar Astrophysics · Physics 2015-05-13 J. Jurcsik , Á. Sódor , B. Szeidl , Zs. Hurta , M. Váradi , K. Posztobányi , K. Vida , G. Hajdu , Zs. Kővári , I. Nagy , L. Molnár , B. Belucz
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