The Galactic center radio source shines below the Compton limit

Details The Galactic center radio source shines below the Compton limit The Galactic center radio source shines below the Compton limit

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...381l..43g&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 381, Nov. 10, 1991, p. L43-L46. Research supported by Los Alamos

Astronomy and Astrophysics

Astronomy

28

Compton Effect, Galactic Nuclei, Interstellar Matter, Radio Sources (Astronomy), Brightness Temperature, Cosmic Plasma, Sagittarius Constellation, Scintillation, Synchrotron Radiation, Very Long Base Interferometry

Scientific paper

Absence of refractive scintillation of Sgr A*, the Galactic center radio source, at 1.3 and 0.8 mm wavelengths places an observational limit of brightness temperature of below 0.5 x 10 exp 12 K on the source. This is less than the maximum brightness of an incoherently synchrotron-emitting plasma, 10 exp 12 K, known as the Compton limit. The refractive scintillations expected, due to strong broadening of the source by the interstellar plasma, are observed by Zhao et al. at decimeter wavelengths. It has proven to be impossible to observe them at 1.3 and 0.8 mm wavelengths over time spans between 0.1 s and 24 hr. Such scintillations are quenched by source size greater than about 0.1 AU, or, equivalently, less than 0.5 x 10 exp 12 K for Sgr A*, at 0.8 mm wavelength. The scintilations would also require fluctuations with scale sizes of 0.1 AU in the scattering plasma, moving across the line of sight at velocities above about 100 km/s. The plasma that scatters Sgr A* satisfies the latter two conditions, and the absence of scintillations is due to the size of the source. This observation strengthens the identification of Sgr A* as a quiescent galactic nucleus.

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