Detection of Sagitarius A* at 330 MHz with the Very Large Array

Details Detection of Sagitarius A* at 330 MHz with the Very Large Array Detection of Sagitarius A* at 330 MHz with the Very Large Array

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.9901n&link_type=abstract

American Astronomical Society Meeting 203, #99.01; Bulletin of the American Astronomical Society, Vol. 35, p.1368

Astronomy and Astrophysics

Astronomy

Scientific paper

We report the detection of Sagitarius A*, the radio source associated with the Milky Way's central ˜ 3 million solar mass black hole, in a high resolution, high sensitivity, 330 MHz Very Large Array image. This is the lowest radio frequency detection to date of this source. Implications for the spectrum, emission processes, and location of Sagittarius A* with the respect to nearby objects are discussed.
Basic research in radio astronomy at the NRL is supported by the Office of Naval Research. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.

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