The kinematically decoupled core of MCG-6-30-15
Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review
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.
Original language | English |
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Title of host publication | Multiwavelength AGN Surveys and Studies |
Number of pages | 4 |
Publisher | cambridge university press (cup) |
Publication date | Jul 2014 |
Edition | S304 |
Pages | 270-273 |
ISBN (Print) | 9781107045248 |
DOIs | |
Publication status | Published - Jul 2014 |
Externally published | Yes |
Series | Proceedings of the International Astronomical Union |
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Number | S304 |
Volume | 9 |
ISSN | 1743-9213 |
- accretion, galaxies: individual(MCG-6-30-15), galaxies: Seyfert, galaxies:active
Research areas
ID: 272400746