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A model for the molecular accretion disk and H2O maser in the nucleus of the galaxy NGC 4258

✍ Scribed by N. S. Babkovskaya; D. A. Varshalovich

Book ID
110143860
Publisher
Springer
Year
2000
Tongue
English
Weight
126 KB
Volume
26
Category
Article
ISSN
1063-7737

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## Abstract We present multi‐frequency simultaneous VLBA observations at 15, 22 and 43 GHz towards the nucleus of the nearby radio galaxy NGC 1052. These three continuum images reveal a double‐sided jet structure, whose relative intensity ratios imply that the jet axis is oriented close to the sky