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most citedStroemgren photometry of Galactic Globular Clusters. I. New Calibrations of the metallicity index

73 citations · 251 across the 16 of their papers we have counts for

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Showing 2007Show all

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astro-ph2007

Metallicity estimates of Galactic Cepheids based on Walraven photometry

S. Pedicelli, J. Lub, J. W. Pel +13

We present new empirical and theoretical calibrations of two photometric metallicity indices based on Walraven photometry. The empirical calibration relies on a sample of 48 Cephei…

astro-ph200740 cited

On the white dwarf cooling sequence of the globular cluster Omega Centauri

A. Calamida, C. E. Corsi, G. Bono +16

We present deep and precise photometry (F435, F625W, F658N) of Omega Cen collected with the Advanced Camera for Surveys (ACS) on board the Hubble Space Telescope (HST). We have ide…

astro-ph2007

On the radial distribution of white dwarfs in the Galactic globular cluster Omega Cen

A. Calamida, C. E. Corsi, G. Bono +14

We present deep and accurate photometry (F435W, F625W, F658N) of the Galactic Globular Cluster Omega Cen collected with the Advanced Camera for Surveys (ACS) on board the Hubble Sp…

astro-ph2007

Stroemgren metallicity calibration: the m1, b-y relation

A. Calamida, G. Bono, P. B. Stetson +15

We performed a new calibration of the Stroemgren metallicity index m1 based on the b-y color of cluster red giant stars. The current Metallicity-Index-Color relation is not linear…

astro-ph200773 cited

Stroemgren photometry of Galactic Globular Clusters. I. New Calibrations of the metallicity index

A. Calamida, G. Bono, P. B. Stetson +15

We present a new calibration of the Stroemgren metallicity index m1 using red giant (RG) stars in 4 globular clusters (GCs:M92,M13,NGC1851,47Tuc) with metallicity ranging from [Fe/…

astro-ph2007

Metallicity distribution of Omega Cen Red Giants based on the Stroemgren m1 metallicity index

A. Calamida, G. Bono, L. M. Freyhammer +6

We adopted uvby Stroemgren photometry to investigate the metallicity distribution of Omega Cen Red Giant (RG) stars. We provided a new empirical calibration of the Stroemgren m1 =…