Intense sub-arcsecond structure in the galactic center

Details Intense sub-arcsecond structure in the galactic center Intense sub-arcsecond structure in the galactic center

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...194..265b&link_type=abstract

Astrophysical Journal, vol. 194, Dec. 1, 1974, pt. 1, p. 265-270.

Astronomy and Astrophysics

Astronomy

193

Fine Structure, Galactic Nuclei, Galactic Radio Waves, Microwave Emission, Radio Sources (Astronomy), Brightness Temperature, Galactic Structure, Graphs (Charts), Ionized Gases, Microwave Interferometers, Milky Way Galaxy, Radiant Flux Density

Scientific paper

The detection of strong radio emission in the direction of the inner 1-pc core of the galactic nucleus is reported. The structure is bright (brightness temperature greater than or about equal to 10,000,000 K), unresolved (angular diameter less than or about equal to 0.1 sec), and distributed within a few seconds of the brightest infrared and radio emission seen previously.

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