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astro-ph20088 cited

Matching the frequency spectrum of PMS stars by means of standard and rotating models

M. Di Criscienzo, P. Ventura, F. D' Antona +3

We applied the ATON code to the computation of detailed grids of standard (non--rotating) and rotating Pre--Main Sequence (PMS) models and computed their adiabatic oscillation spec…

astro-ph2007

NGC 2419: an "intergalactic wanderer" or a simple Galactic Globular Cluster?

M. Di Criscienzo, C. Greco, M. Dall'Ora +8

We have carried out a new photometric study of the remote Galactic globular cluster NGC 2419, using proprietary and archive B,V,I time-series CCD photometry of the cluster, that al…

astro-ph2007

Pulsational models of BL Her stars

M. Di Criscienzo, M. Marconi, F. Caputo +1

We present an updated and homogeneous pulsational scenario for a wide range of stellar parameters typical of BL Her stars i.e., Population II Cepheids with periods shorter than 8 d…

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-ph200741 cited

Synthetic properties of bright metal-poor variables. II. BL Her stars

M. Di Criscienzo, F. Caputo, M. Marconi +1

We investigate the properties of the so-called BL Her stars, i.e., Population II Cepheids with periods shorter than 8 days, using updated pulsation models and evolutionary tracks c…

astro-ph200722 cited

Updated pulsation models for BL Herculis stars

M. Marconi, M. Di Criscienzo

Population II pulsatingvariables play a relevant role both as distance indicators and as tracers of the properties of old stellar populations. In this paper we present an update an…