activity
19952023
most citedIntrinsic Shapes of Molecular Cloud Cores

81 citations · 378 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2023

Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra I. Recovering the fundamental parameters of αEri and βCMi

A. C. Rubio, A. C. Carciofi, P. Ticiani +14

Classical Be stars are fast rotating, near main sequence B-type stars. The rotation and the presence of circumstellar discs profoundly modify the observables of active Be stars. Ou…

astro-ph.SR2023

Non-LTE Monte Carlo Radiative Transfer. III. The thermal properties of Tilted and Warped Be Star Discs

M. W. Suffak, C. E. Jones, A. C. Carciofi +1

We use the three-dimensional Monte Carlo radiative transfer code HDUST to model Be stars where the disc is tilted from the equatorial plane of the star. We compute 128 models acros…

astro-ph.SR2021★ 33 cited

Growth and Dissipation of Be Star Discs in Misaligned Binary Systems

M. Suffak, C. E. Jones, A. C. Carciofi

We use a three-dimensional smoothed particle hydrodynamics code to simulate growth and dissipation of Be star discs in systems where the binary orbit is misaligned with respect to…

nucl-ex2019★ 1 cited

Decay spectroscopy of Sc and Sc to Ti

M. Bowry, C. E. Jones, A. B. Garnsworthy +10

The decay of the isomeric and ground state of Sc to the semi-magic nucleus Ti has been studied using a Ca beam delivered to the GRIFFIN -ray…

astro-ph.SR2017★ 7 cited

Computing the Photometric and Polarimetric Variability of Be Stars

Keegan C. Marr, C. E. Jones, R. J. Halonen

We investigate variations in the linear polarization as well as in the V-band and B-band colour-magnitudes for classical Be star disks. We present two models: disks with enhanced d…

astro-ph.SR2017★ 6 cited

The disk physical conditions of 48 Persei constrained by contemporaneous Hα spectroscopy and interferometry

C. E. Jones, T. A. A. Sigut, B. J. Grzenia +2

We utilize a multi-step modelling process to produce synthetic interferometric and spectroscopic observables, which are then compared to their observed counterparts. Our extensive…