activity
19952017
most citedRR Lyrae Variables in the Globular Cluster M55. The First Evidence for Non Radial Pulsations in RR Lyr Stars

87 citations · 543 across the 55 of their papers we have counts for

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astro-ph2008★ 28 cited

Double mode RR Lyrae stars in Omega Centauri

A. Olech, P. Moskalik

Aim: The aim of this work was to search for double mode pulsators among RR Lyr variables of globular cluster Omega Cen. Methods: We conducted a systematic frequency analysis of CAS…

astro-ph2008★ 10 cited

Curious Variables Experiment (CURVE). CCD photometry of active dwarf nova DI UMa

A. Rutkowski, A. Olech, M. Wiśniewski +3

We report an analysis of photometric behaviour of DI UMa, an extremely active dwarf nova. The observational campaign (completed in 2007) covers five superoutbursts and four normal…

astro-ph2008★ 1 cited

Multiperiodic RR Lyrae Stars in Omega Centauri

P. Moskalik, A. Olech

We have conducted a systematic search for multiperiodic pulsations in the RR Lyrae-type stars of the galactic globular cluster Omega Cen. Secondary periodicities close to the prima…

astro-ph2008★ 1 cited

Curious Variables Experiment (CURVE). RZ LMi - the most active SU UMa star

A. Olech, M. Wisniewski, K. Zloczewski +3

We report extensive photometry of the frequently outbursting dwarf nova RZ Leo Minoris. During two seasons of observations we detected 12 superoutbursts and 7 normal outbursts. The…

astro-ph2008

CURiuos Variables Experiment (CURVE): Variable Stars in the metal-poor Globular Cluster M56

P. Pietrukowicz, A. Olech, P. Kedzierski +3

We have surveyed a 6.5' x 6.5' field centered on the globular cluster M56 (NGC 6779) in search for variable stars. We have detected seven variables, among which two objects are new…

astro-ph2008

Curious Variables Experiment (CURVE). Three Periodicities of BF Ara

A. Olech, A. Rutkowski, A. Schwarzenberg-Czerny

We report CCD photometry of the dwarf nova BF Ara throughout fifteen consecutive nights in quiescence. Light curve in this interval is dominated by a large amplitude around 0.8 mag…