The continuum flux from Sagittarius A* at 222 GHz

Details The continuum flux from Sagittarius A* at 222 GHz The continuum flux from Sagittarius A* at 222 GHz

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...401l..87s&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 401, no. 2, p. L87, L88.

Astronomy and Astrophysics

Astronomy

10

Galactic Nuclei, Milky Way Galaxy, Radio Sources (Astronomy), Emission Spectra, Radiant Flux Density, Sagittarius Constellation

Scientific paper

The 221.9 GHz flux density from Sgr A*, the compact radio source at the center of our Galaxy, has been measured to be 2.4 +/- 0.5 Jy with the OVRO millimeter-wave interferometer. This emission level is well above that seen at lower frequencies, indicating the onset of a different emission component at near-millimeter wavelengths. We also report the possible detection of the supergiant IRS 7 at this frequency.

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