Detection of Sagittarius A at 330 MHz with the Very Large Array

We report the detection of Sagittarius A*, the radio source associated with our Galaxy's central massive black hole, at 330 MHz with the Very Large Array. Implications for the spectrum and emission processes of Sagittarius A* are discussed and several hypothetical geometries of the central regi...

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Published inarXiv.org
Main Authors Nord, Michael E, Lazio, T Joseph W, Kassim, Namir E, Goss, W M, Duric, N
Format Paper
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 08.12.2003
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Summary:We report the detection of Sagittarius A*, the radio source associated with our Galaxy's central massive black hole, at 330 MHz with the Very Large Array. Implications for the spectrum and emission processes of Sagittarius A* are discussed and several hypothetical geometries of the central region are considered.
ISSN:2331-8422
DOI:10.48550/arxiv.0312219