activity
20242026
collaborators

10 papers

astro-ph.SR2026

The Effects of Accretion Feedback on Stellar Evolution in AGN Disks

Alexander J. Dittmann, Matteo Cantiello

Stars embedded in the accretion disks of active galactic nuclei (AGN) can accrete rapidly from their surroundings, dramatically altering their structure and evolution. However, fee…

astro-ph.SR2026

MESA Isochrones and Stellar Tracks. II. Models with alpha-enhanced chemical composition

A Dotter, E Bauer, MJ Park +4

We update and expand the MESA Isochrones and Stellar Tracks (MIST) database to include variations in the alpha-capture elements, specifically [alpha/Fe]=-0.2, 0, +0.2, +0.4, and +0…

astro-ph.HE2025

Pulsational Instability of Quasi-Stars: Interpreting the Variability of Little Red Dots

Matteo Cantiello, Jake B. Hassan, Rosalba Perna +5

The JWST discovery of "Little Red Dots" (LRDs) has revealed a population of compact, red sources at that likely host supermassive black holes (SMBHs). Recent observat…

astro-ph.SR2025

Predicting Stellar Parameters of Massive Stars from Light Curves with Machine Learning

Rachel C. Zhang, Kaze W. K. Wong, Gonzalo Holgado +1

High-resolution spectroscopic measurements of OB stars are important for understanding processes like stellar evolution, but require labor-intensive observations. In contrast, phot…

astro-ph.GA2025

An Extremely Luminous Flare Recorded from a Supermassive Black Hole

Matthew J. Graham, Barry McKernan, K. E. Saavik Ford +17

Since their discovery more than 60 years ago, accreting supermassive black holes in active galactic nuclei (AGN) were recognized as highly variable sources, requiring an extremely…

astro-ph.SR2025

The Growth of the Central Black Holes in Quasi-stars

Jake Hassan, Rosalba Perna, Matteo Cantiello +3

Observations by JWST have confirmed the presence of supermassive black holes (BHs) at redshifts , lending support to scenarios in which BHs experience rapid growth thro…