中文
相关论文

相关论文: Connection between the period and the amplitude of…

200 篇论文

With increasingly accurate data on RR Lyrae stars we find that the Blazhko effect may be a rule rather than an exception. However, we still do not know what is the cause of this mysterious amplitude and phase modulation. In my talk, I…

太阳与恒星天体物理 · 物理学 2011-08-26 Katrien Kolenberg

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…

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

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

In order to benefit from the 4-year unprecedented precision of the Kepler data, we extracted light curves from the pixel photometric data of the Kepler space telescope for 15 Blazhko RR Lyrae stars. For collecting all the flux from a given…

太阳与恒星天体物理 · 物理学 2015-06-22 J. M. Benkő , E. Plachy , R. Szabó , L. Molnár , Z. Kolláth

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…

太阳与恒星天体物理 · 物理学 2015-06-03 R. Szabó , Z. Kolláth , L. Molnár , K. Kolenberg , D. W. Kurtz , WG#13 members

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…

太阳与恒星天体物理 · 物理学 2020-03-10 M. Skarka , Z. Prudil , J. Jurcsik

Recent photometric space missions, such as CoRoT and Kepler revealed that many RR Lyrae stars pulsate -- beyond their main radial pulsation mode -- in low amplitude modes. Space data seem to indicate a clear trend, namely overtone (RRc)…

太阳与恒星天体物理 · 物理学 2015-08-19 J. M. Benkő , R. Szabó

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,…

太阳与恒星天体物理 · 物理学 2010-01-26 Michel Breger

The unprecedented photometric precision along with the quasi-continuous sampling provided by the Kepler space telescope revealed new and unpredicted phenomena that reformed and invigorated RR Lyrae star research. The discovery of period…

太阳与恒星天体物理 · 物理学 2020-11-25 Emese Plachy , Róbert Szabó

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

We analyzed the incidence and properties of RR Lyrae stars that show evidence for amplitude and phase modulation (the so-called Blazhko Effect) in a sample of $\sim$3,000 stars with LINEAR and ZTF light curve data collected during the…

太阳与恒星天体物理 · 物理学 2025-04-09 Ema Donev , Željko Ivezić

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…

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

Pulsations in RR Lyrae stars and classical Cepheids were thought to be relatively simple since they typically pulsate only in one or two radial modes. This picture changes at a closer look when modulation or additional low-amplitude signals…

太阳与恒星天体物理 · 物理学 2023-10-24 H. Netzel

We study the 1.28 million short cadence {\it Kepler} data points (Q5-Q14) for RR Lyrae covering 24 cycles of the Blazhko variation, and more than one half of the 4-year modulation of the Blazhko variation. This very rich data set clearly…

太阳与恒星天体物理 · 物理学 2013-10-03 Robert F. Stellingwerf , James M. Nemec , Pawel Moskalik

Noting the weakest modulation and relatively high metal abundance of the ab-type RR Lyrae star V838 Cyg, we collected the photometric data of this star from several sky surveys to carry out an in-depth analysis. The O-C diagram shows that…

太阳与恒星天体物理 · 物理学 2023-08-04 L. -J. Li , S. -B. Qian , X. -D. Shi , L. -Y. Zhu

A high percentage of the astrophysically important RR Lyrae stars show a periodic amplitude and/or phase modulation of their pulsation cycles. More than a century after its discovery, this "Blazhko effect" still lacks acceptable theoretical…

太阳与恒星天体物理 · 物理学 2009-10-02 Katrien Kolenberg , Stefano Bagnulo

The observations of the photometric space telescopes CoRoT and Kepler show numerous Blazhko RR Lyrae stars which have non-repetitive modulation cycles. The phenomenon can be explained by multi-periodic, stochastic or chaotic processes. From…

太阳与恒星天体物理 · 物理学 2013-07-15 J. M. Benkő , M. Paparó

We search for signs of period doubling in CoRoT RR Lyrae stars. The occurrence of this dynamical effect in modulated RR Lyrae stars might help us to gain more information about the mysterious Blazhko effect. The temporal variability of the…

太阳与恒星天体物理 · 物理学 2014-11-05 R. Szabó , J. M. Benkő , M. Paparó , E. Chapellier , E. Poretti , A. Baglin , W. W. Weiss , K. Kolenberg , E. Guggenberger , J. -F. Le Borgne
‹ 上一页 1 2 3 10 下一页 ›