Astron. Astrophys. 357, 850-870 (2000)

Stellar populations in active galactic nuclei

II. Population synthesis ^*

C. Boisson ¹, M. Joly ¹, J. Moultaka ¹, D. Pelat ¹ and M. Serote Roos <sup>2,1

1</sup> DAEC, Unité associée au CNRS et à l'Université Denis Diderot, Observatoire de Paris, section de Meudon, 92195 Meudon Cedex, France
² Observatório Astronómico de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal

Received 9 August 1999 / Accepted 27 March 2000

Abstract

The relationship of an AGN to its host galaxy is one crucial question in the study of galaxy evolution. We present a method to estimate the stellar contribution in active galactic nuclei. We perform stellar population synthesis in the central regions of a sample of 12 galaxies of different levels of activity: normal galaxies, starburst galaxies, LINERs, Seyfert 2 and Seyfert 1 galaxies. Quantification of the stellar contribution is carried out in the visible range (5000 to 8800 Å) using the equivalent widths of the absorption features throughout the spectrum. The synthesis is done by a variant of the new GPG method (Pelat, 1997). This method, contrary to previous ones, gives a unique solution.

We find quite different stellar populations for the different types of activity, which seems to be indicative of an age sequence. The starburst galaxies present the youngest populations of the sample. The Seyfert 2 nuclei and NGC 1275, a Seyfert 1 with signs of interaction and where young stellar clusters have been found, also show the contribution of a young population, less intense than in the starburst galaxies but metal rich. NGC 3516, a typical Seyfert 1, has a normal population characteristic of galaxies of the same Hubble type and finally the LINERs show the oldest populations in the sample, metal rich, with little star formation still going on.

It is found that a strong CaII triplet, even though these lines are sensitive to gravity, does not imply necessarily a stellar population dominated by supergiant stars.

Key words: galaxies: active galaxies: stellar content galaxies: nuclei galaxies: Seyfert galaxies: starburst

* Based on observations collected at the Canadian-French-Hawaiian Telescope, Hawaii, and Observatoire de Haute Provence, France.

Send offprint requests to: C. Boisson

Correspondence to: catherine.boisson@obspm.fr

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Contents

• 1. Introduction
• 2. The galaxy sample
• 3. The stellar library
• 4. The mathematical method
• 5. Results
  • 5.1. The template galaxies
    • 5.1.1. NGC 3379
    • 5.1.2. NGC 3521
  • 5.2. The starburst galaxies
    • 5.2.1. NGC 3310
    • 5.2.2. He 2-10
  • 5.3. The LINERs
    • 5.3.1. NGC 4278
    • 5.3.2. M 81
    • 5.3.3. NGC 5033
  • 5.4. The Seyfert 2 galaxies
    • 5.4.1. NGC 2110
    • 5.4.2. Mrk 620
    • 5.4.3. Mrk 3
  • 5.5. The Seyfert 1 galaxies
    • 5.5.1. NGC 1275
    • 5.5.2. NGC 3516
• 6. Discussion and conclusions
• Acknowledgements
• References

© European Southern Observatory (ESO) 2000

Online publication: June 5, 2000
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