activity
20242026
collaborators

7 papers

astro-ph.SR2026

Anti-Solar Differential Rotation May Have Revived Magnetic Braking in the Subgiant 31 Aquilae

Travis S. Metcalfe, Jennifer L. van Saders, Thomas R. Ayres +16

Recent observations have shown that sufficiently slow rotation disrupts the organization of large-scale magnetic field in older main-sequence stars, leading to weakened magnetic br…

astro-ph.SR2026

Editorial: Mass and Angular Momentum Transport of Rapidly Rotating Hot Stars

P. A. Scowen, Carol E. Jones, René D. Oudmaijer +2

This dedicated journal collection will present and discuss a variety of science cases that can be used to extend our knowledge of massive stars and the influence of their rapid rot…

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

High energy emission powered by accreting companions of Be/gamma Cas stars

Rina G. Rast, Yael Naze, Jonathan Labadie-Bartz +6

The origin of the hard, bright X-ray emission that defines the gamma Cas analog class of Be stars remains an outstanding question in Be star literature. This work explores the poss…

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…