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Related papers: Blazhko Effect in Double Mode Cepheids

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Detailed knowledge of the variability of classical Cepheids, in particular their modulations and mode composition, provides crucial insight into stellar structure and pulsation. However, tiny modulations of the dominant radial-mode…

Solar and Stellar Astrophysics · Physics 2018-04-25 M. Süveges , R. I. Anderson

V473 Lyrae is the only Galactic Cepheid with confirmed periodic amplitude and phase variations similar to the Blazhko effect observed in RR Lyrae stars. We collected all available photometric data and some radial velocity measurements to…

Solar and Stellar Astrophysics · Physics 2015-06-19 László Molnár , László Szabados

We present a sample of 93 double-mode Cepheids detected in the 2.4 square degree area in the central part of the SMC. 23 stars from the sample pulsate in the fundamental mode and the first overtone while 70 objects are the first and second…

Astrophysics · Physics 2007-05-23 A. Udalski , I. Soszynski , M. Szymanski , M. Kubiak , G. Pietrzynski , P. Wozniak , K. Zebrun

The first detection of the period doubling phenomenon is reported in the Kepler RR Lyrae stars RR Lyr, V808 Cyg and V355 Lyr. Interestingly, all these pulsating stars show Blazhko modulation. The period doubling manifests itself as…

We have analysed Optical Gravitational Lensing Experiment photometry for first overtone classical Cepheids in the Large and Small Magellanic Clouds in search for additional periodicities beyond radial modes. We have used standard…

Solar and Stellar Astrophysics · Physics 2022-12-19 R. Smolec , O. Ziółkowska , M. Ochalik , M. Śniegowska

The origin of the conspicuous amplitude and phase modulation of the RR Lyrae pulsation - known as the Blazhko effect - is still a mystery after more than 100 years of its discovery. With the help of the Kepler space telescope we have…

Solar and Stellar Astrophysics · Physics 2015-06-03 R. Szabó , Z. Kolláth , L. Molnár , K. Kolenberg , D. W. Kurtz , WG#13 members

Until now, double mode Cepheids (or beat Cepheids) were known in the Galaxy, Magellanic Clouds and M33. Curiously, none of more than 2000 Cepheids in M31 was claimed to show two pulsation modes. We conducted a systematic search for double…

Solar and Stellar Astrophysics · Physics 2015-06-16 Radosław Poleski

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

Data on multimode Cepheids from OGLE-III catalog of the LMC Cepheids are confronted with results from model calculations. Models whose radial mode periods are consistent with observation are not always in agreement with published…

Solar and Stellar Astrophysics · Physics 2009-10-02 W. A. Dziembowski , R. Smolec

We present a sample of 76 double-mode Cepheids detected in the 4.5 square degree area in the central part of the LMC. 19 stars from the sample pulsate in the fundamental mode and the first overtone while 57 objects are the first and second…

Astrophysics · Physics 2007-05-23 I. Soszynski , A. Udalski , M. Szymanski , M. Kubiak , G. Pietrzynski , P. Wozniak , K. Zebrun

The importance of Cepheids is well known in many fields of astronomy. Section 2 introduces the Fourier decomposition, a tool to describe quantitatively the light curves of pulsating stars. Sect. 3 shows how an observational result was…

Astrophysics · Physics 2007-05-23 Ennio Poretti

The Blazhko effect is a long term, generally irregular modulation of the light curves that occurs in a sizeable number of RR Lyrae stars. The physical origin of the effect has been a puzzle ever since its discovery over a hundred years ago.…

Solar and Stellar Astrophysics · Physics 2015-05-20 J. Robert Buchler , Zoltan Kollath

We present the hydrodynamic BL Herculis-type models which display a long-term modulation of pulsation amplitudes and phases. The modulation is either strictly periodic or it is quasi-periodic, with the modulation period and modulation…

Solar and Stellar Astrophysics · Physics 2012-09-13 R. Smolec , P. Moskalik

We present a photometric study of two new double-mode Cepheids, pulsating in the first and second overtones modes: V470 Cas and GSC 2901-00089. For the search of the double-mode variability, we used all available observations from the…

Solar and Stellar Astrophysics · Physics 2016-05-05 A. V. Khruslov , A. V. Kusakin

Pulsation period of Cepheids should change as stars evolve through the instability strip. Rates of these changes found by other authors based on the decades-long O-C diagrams show rather good agreement with theoretical predictions. We have…

Solar and Stellar Astrophysics · Physics 2009-01-21 Radoslaw Poleski

We analyse photometry for 138 first overtone Cepheids from the Small Magellanic Cloud, in which Optical Gravitational Lensing Experiment (OGLE) team discovered additional variability with period shorter than first overtone period, and…

Solar and Stellar Astrophysics · Physics 2016-04-05 R. Smolec , M. Sniegowska

We report the discovery of 20 1H/2H and 7 F/1H beat Cepheids in the SMC by the MACHO Project. We utilize the 20 1H/2H stars to determine lightcurve shape for the SMC second-overtone (2H) mode of Cepheid pulsation. We predict, similar to the…

We have conducted a systematic search for multiperiodic pulsations in the RR Lyrae-type stars of the galactic globular cluster Omega Cen. Secondary periodicities close to the primary pulsation frequency have been detected in 17 out of 70…

Astrophysics · Physics 2008-07-17 P. Moskalik , A. Olech

Amplitude and period variations have been detected in almost all types of pulsating stars. Many of these modulations are nearly periodic. In RR Lyrae stars the phenomenon in known as the Blazhko Effect. Because of the observed similarities,…

Solar and Stellar Astrophysics · Physics 2010-01-26 Michel Breger

We present a detailed analysis of the light curves and pulsation properties of First Overtone (FO) Cepheids in the Magellanic Clouds (MCs) obtained using observations and predictions from stellar pulsation models. Multiwavelength…

Astrophysics of Galaxies · Physics 2025-06-19 Kerdaris Kurbah , Shashi M. Kanbur , Sukanta Deb , Anupam Bhardwaj , Mami Deka , Susmita Das , Gautam Bhuyan