activity
20042012
most citedThe Blazhko behaviour of RR Geminorum I - CCD photometric results in 2004

56 citations · 388 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2012★ 14 cited

The light-curve modulation of XY And and UZ Vir - Two Blazhko RR Lyrae stars with additional frequencies

Á. Sódor, G. Hajdu, J. Jurcsik +5

A thorough analysis of multicolour CCD observations of two modulated RRab-type variables, XY And and UZ Vir is presented. These Blazhko stars show relatively simple light-curve mod…

astro-ph.SR2012★ 2 cited

First Results of The Konkoly Blazhko Survey II

Á. Sódor, J. Jurcsik, L. Molnár +17

The two parts of the Konkoly Blazhko Survey (KBS I and II) are introduced. The most important preliminary findings of the second part are presented in comparison to the results of…

astro-ph.SR2010★ 31 cited

Long-term photometric monitoring of Messier 5 variables: II. Blazhko stars

J. Jurcsik, B. Szeidl, C. Clement +2

The light curves of 50 RRab (RR0) stars in M5 collected in Paper I are investigated to detect Blazhko modulation. 18 Blazhko stars are identified, and modulation is suspected in tw…

astro-ph.SR2010★ 30 cited

Long-term photometric monitoring of Messier 5 variables: I. Period changes of RR Lyrae stars

B. Szeid, Zs. Hurta, J. Jurcsik +2

The period changes of 86 M5 RR Lyrae stars have been investigated on a one-hundred-year time base. The published observations have been supplemented by archival Asiago, Konkoly and…

astro-ph.SR2010★ 33 cited

The Multi-periodic Blazhko Modulation of CZ Lacertae

Á. Sódor, J. Jurcsik, B. Szeidl +7

Thorough analysis of the multicolour CCD observations of the RRab-type variable, CZ Lacertae is presented. The observations were carried out in two consecutive observing seasons in…

astro-ph.SR2010★ 13 cited

Four-colour photometry of EY Dra: a study of an ultra-fast rotating active dM1-2e star

K. Vida, K. Oláh, Zs. Kővári +8

We present more than 1000-day long photometry of EY Draconis in BV(RI)C passbands. The changes in the light curve are caused by the spottedness of the rotating surface. Modelling o…