activity
20082025
most citedGrids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)

1.7k citations · 2.7k across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.SR2025

Efficiency of viscous angular momentum transport in dissipating Be binaries

Peter Quigley, Carol E. Jones, Kenneth Gayley +9

Angular momentum transport is a fundamental process shaping the structure, evolution, and lifespans of stars and disks across a wide range of astrophysical systems. Be stars offer…

astro-ph.SR2022★ 3 cited

Angular Momentum Loss Rates in Be Stars Determined by the Viscous Decretion Disc Model

M. R. Ghoreyshi, C. E. Jones, A. Granada

Circumstellar discs around Be stars are formed by the material ejected by the central star. This process removes excess angular momentum from the star as viscosity facilitates the…

astro-ph.SR2022★ 3 cited

Simultaneous J-, H-, K- and L-band spectroscopic observations of galactic Be stars. I. IR atlas

Y. R. Cochetti, M. L. Arias, L. S. Cidale +2

It is already accepted that Be stars are surrounded by circumstellar envelopes, which are mostly compatible with a disc geometry in Keplerian rotation. We aim to obtain a more comp…

astro-ph.GA2021★ 3 cited

Studying the interstellar medium to look for relics of triggered star formation among stellar clusters

S. Paron, A. Granada, M. B. Areal

Evidence of triggered star formation at large spatial scales involving stellar clusters is scarce. We investigate a Galactic region (l=130.0, b=0.35) populated by several open stel…

astro-ph.SR2021★ 7 cited

Intriguing detection of CO molecular emission in a classical Be star

Y. R. Cochetti, M. L. Arias, M. Kraus +4

In the group of B stars with spectroscopic peculiarities, we can find the Be and the B[e] stars. The Be stars are early-type rapid rotators that present, as their principal charact…

astro-ph.SR2017★ 12 cited

Quiescent and active phases in Be stars: A WISE snapshot of young galactic open clusters

A. Granada, C. E. Jones, T. A. A. Sigut +4

Through the modelling of near-infrared photometry of star plus disk systems with the codes BEDISK/BERAY, we successfully describe the WISE photometric characteristics of Be stars i…