We use the data from Gaia Early Data Release 3 (EDR3) to study the kinematic properties of
Milky Way globular clusters. We measure the mean parallaxes and proper motions (PM) for …

We have derived accurate distances to Galactic globular clusters by combining data from the
Gaia Early Data Release 3 (EDR3) with distances based on Hubble Space Telescope (HST) …

The tip of the red giant branch (TRGB) method provides one of the most accurate and
precise means of measuring the distances to nearby galaxies. Here we present a multi …

We have derived the mean proper motions and space velocities of 154 Galactic globular
clusters and the velocity dispersion profiles of 141 globular clusters based on a combination …

We use data from the ESA Gaia mission Early Data Release 3 (EDR3) to measure the
trigonometric parallax of ω Cen, the first high-precision parallax measurement for the most …

Abstract We use Gaia Data Release 2 to determine the mean proper motions for 150 Milky
Way globular clusters (almost the entire known population), with a typical uncertainty of 0.05 …

This is the second paper of a series devoted to presenting an updated release of the BaSTI
(a Bag of Stellar Tracks and Isochrones) stellar model and isochrone library. Following the …

Exploring dark matter via observations of extreme astrophysical environments--defined here
as heavy compact objects such as white dwarfs, neutron stars, and black holes, as well as …

Context. The third Gaia Data Release covers 34 months of data and includes the second
Gaia catalogue of long-period variables (LPVs), with G variability amplitudes larger than 0.1 …

Axion production from astrophysical bodies is a topic in continuous development, because
of theoretical progress in the estimate of stellar emission rates and, especially, because of …