most citedBetelgeuse's Buddy: X-Ray Constraints on the Nature of Ori B

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astro-ph.SR2026

Revealing Optically Hidden Companions to Intermediate-Mass Stripped Stars with Radial Velocities

Alexander Laroche, Maria R. Drout, Ylva Götberg +7

The recent discovery of a population of intermediate-mass helium stars (2-8 ) in the Magellanic Clouds has opened a new observational window into massive binary evol…

astro-ph.SR2026

Disco in the Dust: Reflected light at the bow shock around Betelgeuse's companion explains its observed luminosity

Jared A. Goldberg, Meridith Joyce, Anna J. G. O'Grady +6

Recent detections of Orionis B, the putative companion to Betelgeuse, have been reported using multiple instruments and techniques. These include, most recently, a detect…

astro-ph.SR2026

Hot blue progenitors of stellar-mass black holes

Avishai Gilkis, Eva Laplace, Maria Drout +7

While the connection between massive stars and supernova explosions is well established observationally, the link between massive stars and black hole formation remains elusive. So…

astro-ph.SR2025

The Kinematic Properties of TŻO Candidate HV 11417 with Gaia DR3

Anna J. G. O'Grady

HV 11417 is a candidate Thorne-Żytkow Object, a red supergiant with a neutron star core, located within the Small Magellanic Cloud (SMC). Previous studies have questioned, using Ga…

astro-ph.SR2025

A Spectroscopic Hunt for Post-Red Supergiants in the Large Magellanic Cloud II: Turbulent Line Broadening in the Spectra of LMC Yellow Supergiants

Trevor Z. Dorn-Wallenstein, Kaitlyn M. Chen, Samantha C. Wu +4

Massive stars in the Hertzsprung gap are a mixed population of objects in short-lived evolutionary phases: yellow supergiants (YSGs) evolving towards the red supergiant (RSG) phase…

astro-ph.SR2025★ 4 cited

Betelgeuse's Buddy: X-Ray Constraints on the Nature of Ori B

Anna J. G. O'Grady, Brendan O'Connor, Jared A. Goldberg +8

The d Long Secondary Period of Betelgeuse's optical lightcurve and radial velocity motivated the prediction of a low-mass stellar companion, expected to be at maximal a…

astro-ph.SR2025★ 1 cited

Betelgeuse, Betelgeuse, Betelgeuse, Betel-buddy? Constraints on the dynamical companion to Orionis from HST

Jared A. Goldberg, Anna J. G. O'Grady, Meridith Joyce +10

Recently, two independent analyses have asserted that the cause of the Long Secondary Period (LSP) observed in the variability spectrum of our nearest red supergiant, Betelgeuse ($…