Studies of the central galaxy parsec with high-resolution spatial techniques
This is a multiwavelength study of the centre of the nearest and brightest galaxies at angular scales of a few parsecs. These resolutions, namely <0.1 in average, are currently available across a wide spectral range: in the IR with 8-10m class telescopes and state of the art observational techniques, in the optical-UV with HST, in cm with VLA and
Almudena
Prieto Escudero
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