activity
20242026
collaborators

5 papers

astro-ph.SR2026

Two Be or Not Two Be: A New Companion detection for HD 52244 using HST/FGS

Keefe J. Kamp, Saida M. Caballero-Nieves, Edmund P. Nelan +3

In this paper we present a newly detected companion to the Be star, HD 52244 (B2IVnpe), using the Fine Guidance Sensors (FGSs) on the Hubble Space Telescope (HST). In fall 2021, HS…

astro-ph.SR2026

The Birth of Be Star Disks II. A High-Resolution Spectroscopic Campaign and TESS Observations of an Outburst of the Classical Be star λ Pavonis

Sola S. Nova, Noel D. Richardson, Jonathan Labadie-Bartz +1

Be stars are rapidly-rotating B stars that have shown emission lines originating in a circumstellar disk. The mechanisms that lead to disk formation and dissipation are not known a…

astro-ph.SR2025

TESS Light Curve of the Interacting Binary W Serpentis

Douglas R. Gies, Katherine A. Shepard, Aman Kar +1

The unusual light curve of the massive eclipsing binary W Ser was recently observed with high S/N and fast cadence by the NASA TESS mission. The TESS light curve records two eclips…

astro-ph.SR2025

The birth of Be star disks I. From localized ejection to circularization

J. Labadie-Bartz, A. C. Carciofi, A. C. Rubio +35

Classical Be stars are well known to eject mass, but the details governing the initial distribution and evolution of this matter into a disk are poorly constrained by observations.…

astro-ph.SR2024

An Investigation into the Variability of Luminous Blue Variable Stars with TESS

Becca Spejcher, Noel D. Richardson, Herbert Pablo +3

Luminous Blue Variables (LBVs) are enigmatic, evolved, massive stars. Their variability has been observed to be episodic with large eruptions, along with variations on time-scales…