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The stellar populations of the AGN/Starburst galaxy NGC7582

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 $\sim$ 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 $\sim$ 6 million years ago and has nearly solar metallicity. We also found a Wolf-Rayet cluster.

preprint2010arXivOpen access
T. V. RicciJ. E. SteinerR. B. MenezesA. Garcia-RissmannR. Cid Fernandes
astro-ph.CO
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Open access5 authors1 topic
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T. V. RicciJ. E. SteinerR. B. MenezesA. Garcia-RissmannR. Cid Fernandes

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