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相关论文: The unique dynamical system underlying RR Lyrae pu…

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The recent precise photometric observations and successes of the modelling efforts transformed our picture of the pulsation of RR Lyrae stars. The discovery of additional frequencies and the period doubling phenomenon revealed that a…

太阳与恒星天体物理 · 物理学 2015-06-16 E. Plachy , Z. Kolláth , L. Molnár

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.…

太阳与恒星天体物理 · 物理学 2015-05-20 J. Robert Buchler , Zoltan Kollath

Context. The Blazhko effect, in RR Lyrae type stars, is a century old mystery. Dozens of theory exists, but none have been able to entirely reproduce the observational facts associated to this modulation phenomenon. Existing theory all rely…

太阳与恒星天体物理 · 物理学 2016-10-25 Cyrus Zalian

The Blazhko effect is the conspicuous amplitude and phase modulation of the pulsation of RR Lyrae stars that was discovered in the early 20th century. The field of study of this mysterious modulation has recently been invigorated thanks to…

太阳与恒星天体物理 · 物理学 2015-06-17 R. Szabó

A nonlinear development of radial pulsation instability to a resonant excitation of nonradial modes is studied. The theory covers the cases of axisymmetric (m=0) modes as well as (m,-m) pairs. Adopting a simplified treatment of the mode…

天体物理学 · 物理学 2007-05-23 Rafal M. Nowakowski

We present a highly simplified nonlinear hydrodynamical model to emulate the main observed features of amplitude modulation (commonly known as Blazhko effect) in RR Lyrae stars. The model is based on the assumption that the periodic flow…

太阳与恒星天体物理 · 物理学 2026-05-01 Geza Kovacs

The study of RR Lyrae stars has recently been invigorated thanks to the long, uninterrupted, ultra-precise time series data provided by the Kepler and CoRoT space telescopes. We give a brief overview of the new observational findings…

太阳与恒星天体物理 · 物理学 2015-10-21 R. Szabó , J. M. Benkő , M. Paparó , E. Chapellier , E. Poretti , A. Baglin , W. W. Weiss , K. Kolenberg , E. Guggenberger , J. -F. Le Borgne

We describe a methodology that allows us to follow the pulsational behavior of an RR Lyrae model consistently and automatically along its evolutionary track throughout the whole instability strip. It is based on the powerful amplitude…

天体物理学 · 物理学 2007-05-23 R. Szabo , Z. Kollath , J. R. Buchler

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…

太阳与恒星天体物理 · 物理学 2012-09-13 R. Smolec , P. Moskalik

A significant fraction of RR Lyrae stars exhibits amplitude and/or phase modulation known as the the Blazhko effect. The oscillation spectra suggest that, at least in most of the cases, excitation of nonradial modes in addition to the…

天体物理学 · 物理学 2007-05-23 W. A. Dziembowski , T. T. Mizerski

Steps toward the nature inside RR Lyrae variables can not only improve our understanding of variable stars but also innovate the precision when we use them as tracers to map the structure of the universe. In this work, we develop a…

太阳与恒星天体物理 · 物理学 2021-08-02 Xiao-Wei Duan , Xiao-Dian Chen , Li-Cai Deng , Fan Yang , Chao Liu , Anupam Bhardwaj , Hua-Wei Zhang

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…

太阳与恒星天体物理 · 物理学 2015-06-11 L. Molnár , Z. Kolláth , R. Szabó , E. Plachy

RR Lyrae stars play an important role as distance indicators and stellar population tracers. In this context the construction of accurate pulsation models is crucial to understand the observed properties and to constrain the intrinsic…

太阳与恒星天体物理 · 物理学 2014-11-20 Marcella Marconi

The stellar parameters of RR Lyrae stars vary considerably over a pulsation cycle, and their determination is crucial for stellar modelling. We present a detailed spectroscopic analysis of the pulsating star RR Lyr, the prototype of its…

太阳与恒星天体物理 · 物理学 2015-06-23 L. Fossati , K. Kolenberg , D. V. Shulyak , A. Elmasli , V. Tsymbal , T. G. Barnes , E. Guggenberger , O. Kochukhov

The Blazhko-phenomenon, the modulation of the pulsation of RR Lyrae stars remains one of the most stubborn unsolved problems of stellar pulsation. The recent idea of Stothers proposes that periodic variations in the properties of the…

太阳与恒星天体物理 · 物理学 2015-06-04 L. Molnár , Z. Kolláth , R. Szabó

Preliminary polytropic models of a pulsating star have been constructed using the 3-D Hydrocode SPHC. An embedded Rayleigh-Taylor unstable layer is used to study the interaction of pulsation and turbulence. The possible importance of…

太阳与恒星天体物理 · 物理学 2013-10-03 Robert F. Stellingwerf

Using the novel data set of the MACHO project, we show that three ``Blazhko Effect'' RR Lyrae stars show nearly-pure amplitude modulation of a single pulsation mode. This is strong observational evidence that the ``Oblique Pulsator Model''…

It is shown, that at weakly nonlinear interaction of waves are possible as modes with chaotic dynamics, and with increasing degree of coherence. Conditions are found at which they arise. One of the types of such interaction is decays. The…

混沌动力学 · 物理学 2012-10-26 Vyacheslav Buts , Igor Kovalchuk , Dmytro Tarasov , Alexander Tolstoluzhsky

We investigated period doubling, a well-known phenomenon in dynamical systems, for the first time in RR Lyrae models. These studies provide theoretical background for the recent discovery of period doubling in some Blazhko RR Lyrae stars…

太阳与恒星天体物理 · 物理学 2015-05-27 Z. Kolláth , L. Molnár , R. Szabó

We examined the complete short cadence sample of Kepler RR Lyrae stars to further investigate the recently discovered dynamical effects such as period doubling and additional modes. Here we present the findings on four stars. V450 Lyr may…

太阳与恒星天体物理 · 物理学 2015-06-17 L. Molnár , J. M. Benkő , R. Szabó , Z. Kolláth
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