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20032014
most citedFundamental parameters of RR Lyrae stars from multicolour photometry and Kurucz atmospheric models. I. Theory and practical implementation

5 citations · 19 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2014★ 5 cited

Fundamental parameters of RR Lyrae stars from multicolour photometry and Kurucz atmospheric models -- III. SW And, DH Peg, CU Com, DY Peg

S. Barcza, J. M. Benkő

We report the most comprehensive UBV(RI)_C observations of the bright, radially pulsating field stars SW And, DH Peg, CU Com, DY Peg. Long term variation has been found in the ultr…

astro-ph.SR2011★ 2 cited

Fundamental parameters of RR Lyrae stars from multicolour photometry and Kurucz atmospheric models -- II. Adaptation to double-mode stars

S. Barcza, J. M. Benkő

Our photometric-hydrodynamic method is generalized to determine fundamental parameters of multiperiodic radially pulsating stars. We report 302 UBV(RI)_C Johnson-Kron-Cousins obser…

astro-ph.SR2010★ 5 cited

Fundamental parameters of RR Lyrae stars from multicolour photometry and Kurucz atmospheric models. I. Theory and practical implementation

Szabolcs Barcza

A photometric calibration of Kurucz static model atmospheres is used to obtain the following parameters of RR Lyrae stars: variation of stellar angular radius , effectiv…

astro-ph.SR2010

Fundamental parameters of RR Lyrae stars from multicolour photometry and Kurucz atmospheric models. I. Theory and practical implementation

Szabolcs Barcza

A photometric calibration of Kurucz static model atmospheres is used to obtain parameters of RR Lyrae stars: variation of stellar angular radius , effective temperature…

astro-ph.SR2009★ 3 cited

Five colour photometry of the RRd star V372 Ser

J. M. Benko, S. Barcza

The first UBV(RI)_C time series photometry of the RRd star V372 Ser is presented to determine some parameters of the star. In April, May 2007 2812 U, B, V, R_C, I_C frames were obt…

astro-ph2003★ 4 cited

Distance and mass of pulsating stars from multicolour photometry and atmospheric models

Szabolcs Barcza

For determining distance and mass of pulsating stars a new, purely photometric method is described in which radial velocity observations are not needed. The method is compared with…