Improving black hole accretion treatment in hydrodynamical simulations
Author:
Affiliation:
1. Center for Physical Sciences and Technology , Saulėtekio av. 3, Vilnius LT-10257, Lithuania
2. Astronomical Observatory, Vilnius University , Saulėtekio av. 3, Vilnius LT-10257, Lithuania
Abstract
Funder
Research Council of Lithuania
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stac2330/45497036/stac2330.pdf
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1. NUMERICAL SIMULATIONS OF THE POSSIBLE ORIGIN OF THE TWO SUB-PARSEC SCALE AND COUNTERROTATING STELLAR DISKS AROUND SgrA*
2. Gravitational torque-driven black hole growth and feedback in cosmological simulations
3. ALMA captures feeding and feedback from the active galactic nucleus in NGC 613
4. The photoelectric heating mechanism for very small graphitic grains and polycyclic aromatic hydrocarbons
5. AN IMPROVED DISTANCE AND MASS ESTIMATE FOR SGR A* FROM A MULTISTAR ORBIT ANALYSIS
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