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The kinematically decoupled core of MCG–6-30-15

Published online by Cambridge University Press:  25 July 2014

Sandra I. Raimundo*
Affiliation:
SISSA - International School for Advanced Studies, via Bonomea, 265, 34136 Trieste, Italy email: [email protected]
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Abstract

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The Seyfert galaxy MCG–6-30-15 has recently been observed in the infrared using SINFONI on the VLT, reaching a very high spatial resolution of 0.1 arcsec. This allowed us for the first time to detect a stellar kinematically decoupled core in the inner r < 125 pc of the galaxy. Here we summarise the main theories for the formation of the decoupled core and the implications on the study of this galaxy.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

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