activity
20172021
most citedOn the use of field RR Lyrae as Galactic probes: IV. New insights into and around the Oosterhoff dichotomy

34 citations · 65 across the 3 of their papers we have counts for

collaborators

11 papers

astro-ph.SR202134 cited

On the use of field RR Lyrae as Galactic probes: IV. New insights into and around the Oosterhoff dichotomy

M. Fabrizio, V. F. Braga, J. Crestani +30

We discuss the largest and most homogeneous spectroscopic dataset of field RR Lyrae variables (RRLs) available to date. We estimated abundances using both high-resolution and low-r…

astro-ph.GA2020

Metallicity Distribution of Galactic Halo Field RR Lyrae, and the Effect of Metallicity on their Pulsation Properties

M. Marengo, J. P. Mullen, J. R. Neeley +14

We present our analysis of a large sample (over 150k) of candidate Galactic RR Lyrae (RRL) stars for which we derived high quality photometry at UV, optical and infrared wavelength…

astro-ph.SR2019

On the use of field RR Lyrae as Galactic probes: I. The Oosterhoff dichotomy based on fundamental variables

M. Fabrizio, G. Bono, V. F. Braga +21

We collected a large data set of field RR Lyrae stars (RRLs) by using catalogues already available in the literature and Gaia DR2. We estimated the iron abundances for a sub-sample…

astro-ph.SR2019

Chemical Compositions of Field and Globular Cluster RR~Lyrae Stars: II. omega Centauri

D. Magurno, C. Sneden, G. Bono +21

We present a detailed spectroscopic analysis of RR Lyrae (RRL) variables in the globular cluster NGC 5139 (omega Cen). We collected optical (4580-5330 A), high resolution (R = 34,0…

astro-ph.SR201831 cited

New Near-Infrared light-curve templates for RR Lyrae variables

V. F. Braga, P. B. Stetson, G. Bono +34

We provide homogeneous optical (UBVRI) and near-infrared (JHK) time series photometry for 254 cluster (omega Cen, M4) and field RR Lyrae (RRL) variables. We ended up with more than…

astro-ph.SR2018

unVEil the darknesS of The gAlactic buLgE (VESTALE)

G. Bono, M. Dall'Ora, M. Fabrizio +55

The main aim of this experiment is to provide a complete census of old (t > 10 Gyr, RR Lyrae, type II Cepheids, red horizontal branch), intermediate age (red clump, Miras) and youn…