Published August 2012 | Version v1
Journal article

THE ALL-SKY GEOS RR Lyr SURVEY WITH THE TAROT TELESCOPES: ANALYSIS OF THE BLAZHKO EFFECT

  • 1. Université de Toulouse, UPS-OMP, IRAP, 31400 Toulouse (France)
  • 2. ARTEMIS, Université Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, Nice (France)
  • 3. American Association of Variable Star Observers (AAVSO), 49 Bay State Rd., Cambridge, MA 02138 (United States)
  • 4. Groupe Européen d'Observations Stellaires (GEOS), 23 Parc de Levesville, 28300 Bailleau l'Evêque (France)
  • 5. Bundesdeutsche Arbeitsgemeinschaft für Veränderliche Sterne e.V. (BAV), Munsterdamm 90, 12169 Berlin (Germany)
  • 6. Observatoire Chante-Perdrix, 04150 Banon (France)
  • 7. Agrupació Astronòmica de Sabadell (AAS), Apartat de Correus, 50, 08200 Sabadell, Barcelona (Spain)

Description

We used the GEOS database to study the Blazhko effect of galactic RRab stars. The database is continuously enriched by maxima supplied by amateur astronomers and by a dedicated survey by means of the two TAROT robotic telescopes. The same value of the Blazhko period is observed at different values of the pulsation periods and different values of the Blazhko periods are observed at the same value of the pulsation period. There are clues suggesting that the Blazhko effect is changing from one cycle to the next. The secular changes in the pulsation and Blazhko periods of Z CVn are anticorrelated. The diagrams of magnitudes against phases of the maxima clearly show that the light curves of Blazhko variables can be explained as modulated signals, both in amplitude and in frequency. The closed curves describing the Blazhko cycles in such diagrams have different shapes, reflecting the phase shifts between the epochs of the brightest maximum and the maximum O – C. Our sample shows that both clockwise and counterclockwise directions are possible for similar shapes. The improved observational knowledge of the Blazhko effect, in addition to some peculiarities of the light curves, has yet to be explained by a satisfactory physical mechanism.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-6256/144/2/39

Additional details

Identifiers

Publishing Information

Journal Title
Astronomical Journal (New York, N.Y. Online)
Journal Volume
144
Journal Issue
2
Journal Page Range
[15 p.]
ISSN
1538-3881

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43123298
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
AMPLITUDES; ASTRONOMY; ASTROPHYSICS; DIAGRAMS; LIBRARIES; PHASE SHIFT; PULSATIONS; SHAPE; SIGNALS; STAR EVOLUTION; TELESCOPES; VARIABLE STARS; VISIBLE RADIATION
Descriptors DEC
ELECTROMAGNETIC RADIATION; EVOLUTION; INFORMATION; PHYSICS; RADIATIONS; STARS