Abstract
We demonstrate that there is only one physical process required to explain the spectrum and the variability of the radio source at the dynamical center of our Galaxy, Sgr A*, in the frequency range from =~1 to =~1000 GHz, namely optically thin synchrotron radiation that is emitted from a population of relativistic electrons. We attribute the observed variability to variable energy input from an accretion disk around Sgr A* into the acceleration of the electrons.
Dokumententyp: | Zeitschriftenartikel |
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Publikationsform: | Publisher's Version |
Keywords: | accretion disks; electron plasma; radio astronomy; radio sources (astronomy); radio spectra; relativistic electron beams; synchrotron radiation; variability; galactic bulge; magnetohydrodynamics; particle acceleration; astrophysics; acceleration of particles; accretion; accretion disks; magnetohydrodynamics (mhd); galaxy: center; radio continuum: galaxies; astrophysics |
Fakultät: | Physik |
Themengebiete: | 500 Naturwissenschaften und Mathematik > 520 Astronomie
500 Naturwissenschaften und Mathematik > 530 Physik |
ISSN: | 0004-6361 |
Sprache: | Englisch |
Dokumenten ID: | 76637 |
Datum der Veröffentlichung auf Open Access LMU: | 21. Jul. 2021, 14:20 |
Letzte Änderungen: | 21. Jul. 2021, 14:20 |