Peer-reviewedPublisher termsAstronomy & Astrophysics
Chaotic accretion can (still) explain early supermassive black hole growth
Related
- BlackHoleWeather – Spin-coupled chaotic cold accretion across the meso scale: Kinematics and variability
- Constraining Supermassive Black Hole Seeding and Accretion via Occupation Fractions and Mass-Weighted Distributions
- Magnetized Accretion Flows with Low Angular Momentum Around Supermassive Black Holes
- Disk Structure May Determine AGN Variability and Explain the Accretion Disk Size Problem: No Broad Line Region Required
- Quantifying collision-driven mass loss in supermassive star formation: the role of stellar structure and accretion
BibTeX
@article{zubovas2026chaotic,
title = {{Chaotic accretion can (still) explain early supermassive black hole growth}},
author = {K. Zubovas and M. Tartėnas},
journal = {Astronomy \& Astrophysics},
year = {2026},
month = oct,
doi = {10.1051/0004-6361/202558523},
url = {https://www.aanda.org/10.1051/0004-6361/202558523},
}
RIS
TY - JOUR
TI - Chaotic accretion can (still) explain early supermassive black hole growth
AU - K. Zubovas
AU - M. Tartėnas
PY - 2026
DA - 2026/10/22
JO - Astronomy & Astrophysics
DO - 10.1051/0004-6361/202558523
UR - https://www.aanda.org/10.1051/0004-6361/202558523
SN - 0004-6361
SN - 1432-0746
ER -