Be star
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- Black Hole That Doesn't Emit X-Rays Discovered Near Massive Star 16 January 2014, by Bob Yirka
- A Representative Sample of Be Stars V
- X-Ray Pulsars Sgrs Axps Magnetars RRATS Grbs X-Ray Pulsars • We Have Seen How Radio Pulsars Are Powered by the Rotational Kinetic Energy of the Neutron Star
- Rotation in the ZAMS: Be and Bn Stars J
- The Discovery of a Transient Magnetar
- New Herbig Ae/Be Stars Confirmed Via High-Resolution Optical Spectroscopy
- DENSITY and VELOCITY STRUCTURE of the Be STAR EQUATORIAL DISK in the BINARY LS I +61 303, a PROBABLE MICROQUASAR P
- 50 Years Ago 100 Years
- Black Hole Educator's Guide
- Arxiv:1004.0949V2
- On the Population of Galactic Luminous Blue Variables
- Session 1: Stellar Winds, Diagnostics Across the Electromagnetic Spectrum
- Measuring the Masses of Neutron Stars
- Advanced Astroinformatics for Variable Star Classification by Kyle
- What X-Rays Could Tell Us About Gamma-Ray Burst & Magnetar
- Spin-Up of Be Stars in the Pre-Main Sequence Phase
- The First Black Hole Orbiting a Be Star
- Spectroscopy and Interferometry of the Winds of Luminous Blue Variables