No CrossRef data available.
Article contents
The stellar populations of the AGN/Starburst galaxy NGC7582
Published online by Cambridge University Press: 13 April 2010
Abstract
NGC 7582 is defined as a Starburst/AGN galaxy, since its optical and X-Ray spectra reveal both characteristics. In this work, we show the results of a stellar population modeling in a datacube taken with the Gemini South telescope. We found that ~ 90% of the light in the field of view is emitted by stars that are less than 1 billion years old. A strong burst occurred about ~ 6 million years ago and has nearly solar metallicity. We also found a Wolf-Rayet cluster.
- Type
- Poster Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 416 - 417
- Copyright
- Copyright © International Astronomical Union 2010