FIRST DETECTION OF MULTI-SHOCKS IN RR LYRAE STARS FROM ANTARCTICA: A POSSIBLE EXPLANATION OF THE BLAZHKO EFFECT

2014 ◽  
Vol 148 (5) ◽  
pp. 88 ◽  
Author(s):  
M. Chadid ◽  
J. Vernin ◽  
G. Preston ◽  
C. Zalian ◽  
C. Pouzenc ◽  
...  
1995 ◽  
Vol 155 ◽  
pp. 42-43
Author(s):  
Hiromoto Shibahashi ◽  
Masao Takata

AbstractBy assuming that the RR Lyrae stars have fairly strong dipole magnetic fields with the symmetry axis oblique to the rotation axis of the star, we show that the oscillation mode which would be a pure radial oscillation in absence of the magnetic field has a quadrupole component, which is axisymmetric with respect to the magnetic axis. The aspect angle of the quadrupole component changes due to the stellar rotation, and this apparent variation is interpreted as the Blazhko effect in RR Lyrae stars.


2013 ◽  
Vol 9 (S301) ◽  
pp. 241-248
Author(s):  
Róbert Szabó

AbstractThe 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 the space photometric missions providing long, uninterrupted, ultra-precise time-series data. In this paper I give a brief overview of the new observational findings related to the Blazhko effect, such as extreme modulations, irregular modulation cycles and additional periodicities. I argue that these findings together with dedicated ground-based efforts provide us now with a fairly complete picture and a good starting point to theoretical investigations. Indeed, new, unpredicted dynamical phenomena have been discovered in Blazhko RR Lyrae stars, such as period doubling, high-order resonances, three-mode pulsation and low-dimensional chaos. These led to the proposal of a new explanation to this century-old enigma, namely a high-order resonance between radial modes. Along these lines I present the latest efforts and advances from the theoretical point of view. Lastly, amplitude variations in Cepheids are discussed.


2000 ◽  
Vol 176 ◽  
pp. 291-298 ◽  
Author(s):  
D. W. Kurtz ◽  
C. Alcock ◽  
R. A. Allsman ◽  
D. Alves ◽  
T. S. Axelrod ◽  
...  

AbstractWe present the first results of the analysis of 22 Blazhko stars. We find: 1) Blazhko RRab stars that are nearly pure amplitude modulators; 2) Blazhko RRab stars that have both amplitude and phase modulation; 3) A Blazhko RRab star that has an abrupt period change; 4) Proof of the Blazhko effect in RRc stars. Our data show the character of the amplitude and phase modulations of the light curves over the Blazhko cycles far better than has been previously possible.


2010 ◽  
Vol 409 (3) ◽  
pp. 1244-1252 ◽  
Author(s):  
R. Szabó ◽  
Z. Kolláth ◽  
L. Molnár ◽  
K. Kolenberg ◽  
D. W. Kurtz ◽  
...  

2011 ◽  
Vol 731 (1) ◽  
pp. 24 ◽  
Author(s):  
J. Robert Buchler ◽  
Zoltán Kolláth

2006 ◽  
Vol 652 (1) ◽  
pp. 643-649 ◽  
Author(s):  
Richard B. Stothers

2000 ◽  
Vol 176 ◽  
pp. 299-306 ◽  
Author(s):  
Hiromoto Shibahashi

AbstractBy assuming that RR Lyrae stars have fairly strong dipole magnetic fields with symmetry axis oblique to the rotation axis of the star, I show that the oscillation mode which would be a pure radial oscillation in absence of the magnetic field has a quadrupole component, whose symmetry axis coincides with the magnetic axis. The aspect angle of the quadrupole component changes due to the stellar rotation, and this apparent amplitude variation is interpreted as the Blazhko effect in RR Lyrae stars. It is shown that, in the case of off-axis magnetic field, phase modulation is expected. I list up some theoretical predictions based on this model, which would observationally examine this hypothesis.


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