activity
20242026
collaborators

9 papers

astro-ph.SR2026

The birth of Be star disks III. SPH models of localised mass ejections

A. C. Rubio, A. C. Carciofi, D. Baade +4

Classical Be stars exhibit mass ejection events that feed their viscous decretion disks. Recent TESS space photometry and simultaneous spectroscopy revealed that these flickers are…

astro-ph.SR2026

Constraints on Binarity for the Extreme Oe Variable Star AzV 493

M. S. Oey, Irene Vargas-Salazar, Edmund Hodges-Kluck +6

The extreme Oe star AzV 493 is known to show unusual photometric and spectroscopic variability that suggest the presence of an unseen companion in a highly eccentric and long-perio…

astro-ph.SR2025

Dynamical Masses and Radiative Transfer Modeling of HD 698: a Be Binary in Evolutionary Transition

Ilfa A. Gabitova, Alex C. Carciofi, Tajan H. de Amorim +13

We present a detailed analysis of the early post-mass-transfer binary HD 698 (V742 Cas) combining high-resolution optical spectroscopy, long-baseline interferometry, and radiative-…

astro-ph.SR2025

Exploring the binary origin of B and Be rapid rotators

Jonathan Labadie-Bartz, Mark Suffak, Carol Jones +8

Observational evidence has continued to mount that a significant fraction of rapidly rotating early-B type stars are products of binary mass transfer. However, very few mid- and la…

astro-ph.SR2025

Predicted observational effects of rapid rotation for Be stars

Rina G. Rast, Carol E. Jones, Mark W. Suffak +6

We conduct a systematic study on the effects of rapid rotation on predicted Be star observables. We use the three-dimensional Monte Carlo radiative transfer code, \textsc{hdust}, t…

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…