activity
20032009
most citedClassical Cepheid Pulsation Models. XI. Effects of convection and chemical composition on the Period-Luminosity and Period-Wesenheit relations

72 citations · 205 across the 6 of their papers we have counts for

collaborators

11 papers

astro-ph.SR200922 cited

On the stellar content of the starburst galaxy IC10

N. Sanna, G. Bono, P. B. Stetson +17

We investigate the stellar content of the starburst dwarf galaxy IC10 using accurate and deep optical data collected with the Advanced Camera for Surveys and with the Wide Field Pl…

astro-ph.GA200919 cited

On the radial distribution of horizontal branch stars in ngc2808

G. Iannicola, M. Monelli, G. Bono +17

We present accurate new ultraviolet and optical BVI photometry for the Galactic globular cluster ngc2808, based on both ground-based and archival HST imagery. From this we have sel…

astro-ph20082 cited

MAD@VLT: Deep into the Madding Crowd of Omega Centauri

G. Bono, A. Calamida, C. E. Corsi +18

We present deep and accurate Near-Infrared (NIR) photometry of the Galactic Globular Cluster (GC) Omega Cen. Data were collected using the Multi-Conjugate Adaptive Optics Demonstra…

astro-ph200752 cited

RR Lyrae stars in Galactic globular clusters. VI. The Period-Amplitude relation

G. Bono, F. Caputo, M. Di Criscienzo

We compare theory and observations for fundamental RR Lyrae in the solar neighborhood and in both Oosterhoff type I (OoI) and type II (OoII) Galactic globular clusters (GGCs). The…

astro-ph200772 cited

Classical Cepheid Pulsation Models. XI. Effects of convection and chemical composition on the Period-Luminosity and Period-Wesenheit relations

G. Fiorentino, M. Marconi, I. Musella +1

In spite of the relevance of Classical Cepheids as primary distance indicators, a general consensus on the dependence of the Period-Luminosity (PL) relation on the Cepheid chemical…

astro-ph200638 cited

Synthetic properties of bright metal-poor variables. I. "Anomalous" Cepheids

G. Fiorentino, M. Limongi, F. Caputo +1

We present new grids of evolutionary models for the so-colled ``Anomalous'' Cepheids (ACs), adopting Z=0.0001 and various assumptions on the progenitor mass and mass-loss efficienc…