The Structure and Variability of Sagittarius A*: Zooming in to the Supermassive Black Hole at the Galactic Center
Ye‐Fei Yuan, Jun‐Hui Zhao
Abstract
Open-access reader
Ye‐Fei Yuan, Jun‐Hui Zhao
Abstract
Open-access reader
The Galactic center provides a unique astrophysical laboratory for us to study various astrophysical processes. In this paper, we review and outline the latest results from observations of Sgr~A$^*$ in terms of source structure and variations in flux density. Sgr~A$^*$ phenomenon represents a typical case of low radiative efficiency accretion flow surrounding a supermassive black hole in low luminosity AGNs. Many pending astrophysical problems found from observations of Sgr A$^*$ have challenged the existing astrophysical theories. Current theoretical models of Sgr A$^*$ are also reviewed.
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The Galactic center provides a unique astrophysical laboratory for us to study various astrophysical processes. In this paper, we review and outline the latest results from observations of Sgr~A$^*$ in terms of source structure and variations in flux density. Sgr~A$^*$ phenomenon represents a typical case of low radiative efficiency accretion flow surrounding a supermassive black hole in low luminosity AGNs. Many pending astrophysical problems found from observations of Sgr A$^*$ have challenged the existing astrophysical theories. Current theoretical models of Sgr A$^*$ are also reviewed.
Key concepts: Supermassive black hole, Physics, Galactic Center, Astrophysics, Sagittarius A*, Intermediate-mass black hole, Accretion (finance), Astronomy