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Related papers: Low-dimensional chaos in RR Lyrae models

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We demonstrate how, with a purely empirical analysis of the irregular lightcurve data, one can extract a great deal of information about the stellar pulsation mechanism. An application to R Sct thus shows that the irregular lightcurve is…

Astrophysics · Physics 2016-01-27 J. Robert Buchler , Zoltan Kollath

We analyzed the Long Cadence photometry of 4 first overtone RR Lyr-type stars (RRc stars) observed by the KEPLER telescope. All studied variables are multiperiodic. The strongest secondary peak appears for f_2/f_1 = 1.58-1.63, or P_2/P_1 =…

Solar and Stellar Astrophysics · Physics 2012-08-22 P. Moskalik , R. Smolec , K. Kolenberg , J. Nemec , A. Kunder , M. Chadid , G. Kopacki , R. Szabó , KEPLER WG#13 members

For the first time connection between the pulsation and modulation properties of RR Lyrae stars has been detected. Based on the available data it is found that the possible range of the modulation frequencies, i.e, the possible maximum…

Astrophysics · Physics 2007-05-23 Johanna Jurcsik , Béla Szeidl , Andrea Nagy , Ádám Sódor

We report the discovery of a new group of double-periodic RR Lyrae stars from the analysis of the OGLE-IV Galactic bulge photometry. In 11 stars identified in the OGLE catalog as first overtone pulsators (RRc stars) we detect additional…

Solar and Stellar Astrophysics · Physics 2015-05-14 H. Netzel , R. Smolec , W. Dziembowski

Three dimensional hydrodynamic simulations of full amplitude RR Lyrae stars have been computed for several models across the instability strip. The three dimensional nature of the calculations allows convection to be treated without…

Solar and Stellar Astrophysics · Physics 2015-02-11 Christopher M. Geroux , Robert G. Deupree

Aim: The aim of this work was to search for double mode pulsators among RR Lyr variables of globular cluster Omega Cen. Methods: We conducted a systematic frequency analysis of CASE photometry of Omega Cen RR Lyr stars. We searched for…

Astrophysics · Physics 2009-11-13 A. Olech , P. Moskalik

Spatio-temporal dynamics of a deterministic three-level cellular automaton (TLCA) of Zykov-Mikhailov type (Sov. Phys. - Dokl., 1986, Vol.31, No.1, P.51) is studied numerically. Evolution of spatial structures is investigated both for the…

Other Condensed Matter · Physics 2007-05-23 S. D. Makovetskiy , D. N. Makovetskii

Frequency analysis of more than 300 stars of the OGLE database on Sculptor galaxy has led to the discovery of 18 double-mode RR Lyrae (RRd) variables. This yields a 20% incidence rate for double-mode pulsation among the variables previously…

Astrophysics · Physics 2009-11-06 G. Kovacs

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 the first results of our analyses of selected RR Lyrae stars for which data have been obtained by the Kepler Mission. As expected, we find a significant fraction of the RRab stars to show the Blazhko effect, a still unexplained…

Highly precise and nearly uninterrupted optical photometry of the RR Lyrae star AQ Leo was obtained with the MOST (Microvariability & Oscillations of STars) satellite over 34.4 days in February-March 2005. AQ Leo was the first known…

Strange modes have been found in the radial spectrum of many luminous stars, most recently in Cepheids and RR Lyrae. We show that there is nothing strange about these modes -- they must exist even in the adiabatic limit. With a change of…

Astrophysics · Physics 2008-02-03 J. R. Buchler , P. A. Yecko , Z. Kollath

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

The classic problem of detection of periodic signals in the presence of noise becomes much more challenging if the observation times are themselves periodic, contain large gaps, or consist of data from several different instruments. For RR…

Solar and Stellar Astrophysics · Physics 2011-08-26 Robert F. Stellingwerf

The r-modes of neutron stars can be driven unstable by gravitational radiation. While linear perturbation theory predicts the existence of this instability, linear theory can't provide any information about the nonlinear development of the…

Astrophysics · Physics 2009-11-07 Sharon M. Morsink

Globular clusters offer a powerful way to test the properties of stellar populations and the late stages of low-mass stellar evolution. In this paper we study oscillating giant stars and overtone RR Lyrae-type pulsators in the nearest…

Solar and Stellar Astrophysics · Physics 2025-10-15 László Molnár , Henryka Netzel , Madeline Howell , Csilla Kalup , Meridith Joyce

During intensive/comparative studies with Preston's spectroscopic works (1961, 1962, 1964 & 1965) on RR Lyrae atmospheric phenomena, I unexpectedly found the existence of hypersonic shock waves (Chadid 1996 & 2008), that are strongly…

Solar and Stellar Astrophysics · Physics 2011-08-30 Merieme Chadid

The CoRoT satellite supplied the scientific community with a huge data base of variable stars. Among them the RR Lyrae stars have intensively been discussed in numerous papers in the last few years, but the latest runs have not been checked…

Solar and Stellar Astrophysics · Physics 2016-08-31 J. M. Benkő , R. Szabó , A. Derekas , Á. Sódor

We study the dynamical properties of a broad class of high-dimensional random dynamical systems exhibiting chaotic as well as fixed point and periodic attractors. We consider cases in which attractors can co-exists in some regions of the…

Disordered Systems and Neural Networks · Physics 2026-03-02 Samantha J. Fournier , Pierfrancesco Urbani

Many dynamical systems of different complexity, e.g. 1D logistic map, the Lorentz equations, or real phenomena, like turbulent convection, show chaotic behaviour. Despite huge differences, the dynamical scenarios for these systems are…

Solar and Stellar Astrophysics · Physics 2014-03-24 R. Smolec , P. Moskalik
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