activity
20142019
most citedProper motions and kinematics of selected bulge globular clusters

62 citations · 233 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2019★ 58 cited

Modelling Double Neutron Stars: Radio and Gravitational Waves

Debatri Chattopadhyay, Simon Stevenson, Jarrod R. Hurley +2

We have implemented prescriptions for modelling pulsars in the rapid binary population synthesis code COMPAS. We perform a detailed analysis of the double neutron star (DNS) popula…

astro-ph.GA2019★ 9 cited

A MUSE study of the inner bulge globular cluster Terzan 9: a fossil record in the Galaxy

H. Ernandes, B. Dias, B. Barbuy +5

Context. Moderately metal-poor inner bulge globular clusters are relics of a generation of long-lived stars that formed in the early Galaxy. Terzan 9, projected at 4d 12 from the G…

astro-ph.EP2019

The Search for Living Worlds and the Connection to Our Cosmic Origins

M. A. Barstow, S. Aigrain, J. Barstow +24

One of the most exciting scientific challenges is to detect Earth-like planets in the habitable zones of other stars in the galaxy and search for evidence of life. The ability to o…

astro-ph.SR2018★ 33 cited

High-resolution abundance analysis of four red giants in the globular cluster NGC 6558

B. Barbuy, L. Muniz, S. Ortolani +8

NGC 6558 is a bulge globular cluster with a blue horizontal branch (BHB), combined with a metallicity of [Fe/H]~-1.0. It is similar to HP 1 and NGC 6522, which could be among the o…

astro-ph.GA2018★ 30 cited

Orbits of selected globular clusters in the Galactic bulge

A. Pérez-Villegas, L. Rossi, S. Ortolani +3

We present orbit analysis for a sample of 8 inner bulge globular clusters, together with one reference halo object. We used proper motion values derived from long time base CCD dat…

astro-ph.GA2016★ 27 cited

Evolution of star cluster systems in isolated galaxies: first results from direct -body simulations

L. J. Rossi, K. Bekki, J. R. Hurley

The evolution of star clusters is largely affected by the tidal field generated by the host galaxy. It is thus in principle expected that under the assumption of an "universal" ini…