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

Preprint

9 December 2003

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0312219

Abstract

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.

Keywords

DETECTION OF SAGITTARIUS
RADIO SOURCE
LARGE ARRAY
GEOMETRIES
BLACK HOLE
GALAXY'S

All Related Versions

Version 1, 2003-12-09, ArXiv
Published version: The Astrophysical Journal, 601 (1), L51.

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