Multistructured Accretion Flow of Sgr A*. II. Signatures of a Cool Accretion Disk in Hydrodynamic Simulations of Stellar Winds

Multistructured Accretion Flow of Sgr A*. II. Signatures of a Cool Accretion Disk in Hydrodynamic Simulations of Stellar Winds

Hydrodynamic simulations of the stellar winds from Wolf–Rayet stars within the Galactic center can provide predictions for the X-ray spectrum of the supermassive black hole Sgr A*. Herein, we present results from updated smooth particle hydrodynamics simulations, building on the architecture of Cuad...

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Bibliographic Details
Main Authors: Mayura Balakrishnan, Christopher M. P. Russell, Lia Corrales, Diego Calderón, Jorge Cuadra, Daryl Haggard, Sera Markoff, Joey Neilsen, Michael Nowak, Q. Daniel Wang, Frederick Baganoff
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Supermassive black holes
Galactic center
Hydrodynamical simulations
Wolf-Rayet stars
Online Access:https://doi.org/10.3847/1538-4357/ad6866

Internet

https://doi.org/10.3847/1538-4357/ad6866

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