activity
20242026
collaborators

5 papers

astro-ph.SR2026

Fading into darkness: A weak mass ejection and low-efficiency fallback accompanying black hole formation in M31-2014-DS1

Kishalay De, Morgan MacLeod, Jacob E. Jencson +10

Stellar-mass black holes (BHs) can form from the near-complete collapse of massive stars, causing them to abruptly disappear. The star M31-2014-DS1 in the Andromeda galaxy was repo…

astro-ph.HE2026

Disappearance of a massive star in the Andromeda Galaxy due to formation of a black hole

Kishalay De, Morgan MacLeod, Jacob E. Jencson +11

When a massive star reaches the end of its lifetime, its core collapses and releases neutrinos that drive a shock into the outer layers (stellar envelope). A sufficiently strong sh…

astro-ph.EP2025

On the coincidence between the close passage of HD7977 and the Pliocene-Pleistocene transition

Zhuoya Cao, Abraham Loeb, Morgan MacLeod

The Oort Cloud's dynamical evolution is significantly influenced by both the galactic tide and stellar flybys. This study investigates the particular case of HD7977's close encount…

astro-ph.SR2025

Tidal Amplitudes in the Magellanic Cloud Population of Heartbeat Stars

Morgan MacLeod, Abraham Loeb

Heartbeat (HB) stars exhibit pulses in their light curves once per orbit due to ellipsoidal distortions from strong tides at periapse. We analyze the population of HB stars in the…

astro-ph.SR2024

Radial Velocity and Astrometric Evidence for a Close Companion to Betelgeuse

Morgan MacLeod, Sarah Blunt, Robert J. De Rosa +10

We examine a century of radial velocity, visual magnitude, and astrometric observations of the nearest red supergiant, Betelgeuse, in order to reexamine the century-old assertion t…