Blazhko effect in Cepheids and RR Lyr stars

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In collaboration with - K. Kolenberg – co-chair of KASC <strong>RR</strong>L & Cep WG + other members of KASC (Kepler Asteroseismic Science Consortium) - Z. Kolláth, J. Benkő, L. Molnár, E. Plachy + other KIK-members, Kepler Investigations at Konkoly Observatory http:www.konkoly.hu/KIK/
Acknowledgements Acknowledg<strong>in</strong>g the support from - IAU - the Lendület Young Researchers' Program - the Bolyai Scholarship of the Hungarian Academy of Sciences - Hungarian OTKA grant K83790 - HUMAN MB08C 81013 grant of the MAG Zrt - KTIA URKUT_10-1-2011-0019 grant - EU FP7 IRSES/ASK grant no. 269194
Page 1 and 2: Blazhko effect in Cepheids and RR L
Page 3 and 4: RR Lyrae stars and the Blazhko effe
Page 5 and 6: The beginning On the changes in the
Page 7 and 8: Kepler and the Blazhko effect Quasi
Page 9 and 10: Extreme modulation: V445 Lyr aka KI
Page 11 and 12: Multiple modulations longest P BL s
Page 13 and 14: Period doubling in RR Lyr (Q1+Q2)
Page 15 and 16: Period doubling in CoRoT data V1127
Page 17 and 18: Hydro results Kolláth, Molnár, Sz
Page 19 and 20: A new explanation for the Blazhko e
Page 21 and 22: Bifurcation cascades Bifurcation-ca
Page 23 and 24: Period-6 state, 3:4 resonance RR Ly
Page 25 and 26: Cepheids Amplitude variation in Cep
Page 27 and 28: Future
Page 29 and 30: Photometry EU: PLATO (PLAnetary Tra
Page 31 and 32: Spectroscopy Detection of He I and
Page 33 and 34: Blazhko effect - proposed mechanism
Page 35 and 36: Conclusions - Space photometry revi
Page 37: Thank you
Page 40 and 41: Nonlinear 'diagnostic' diagram Blue

Blazhko effect in Cepheids and RR Lyr stars

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