Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-04-18
Mon.Not.Roy.Astron.Soc. 359 (2005) 1237-1249
Astronomy and Astrophysics
Astrophysics
14 pages, 11 figures
Scientific paper
10.1111/j.1365-2966.2005.09003.x
We present a method for generating virtual observations from smoothed-particle-hydrodynamics (SPH) simulations. This method includes stellar population synthesis models and the reprocessing of starlight by dust to produce realistic galaxy images. We apply this method and simulate the merging of two identical giant Sa galaxies. The merger remnant is an elliptical galaxy. The merger concentrates the gas content of the two galaxies into the nuclear region. The gas that flows into the nuclear region refuels the central black holes of the merging galaxies. We follow the refuelling of the black holes during the merger semi-analytically. In the simulation presented in this article, the black holes grow from 3 x 10^7 to 1.8X 10^8 Solar masses, with a peak AGN luminosity of M_B ~ -23.7. We study how the morphological and spectral properties of the system evolve during the merger and work out the predictions of this scenario for the properties of host galaxies during the active phase. The peak of AGN activity coincides with the merging of the two galactic nuclei and occurs at a stage when the remnant looks like a lenticular galaxy. The simulation predicts the formation of a circumnuclear starburst ring/dusty torus with an opening angle of 30-40 degrees and made of clouds with n_H=10^24 cm^-2. The average optical depth of the torus is quite high, but the obscuring medium is patchy, so that there still exist lines of sight where the AGN is visible in a nearly edge-on view. For the same reason, there are lines of sight where the AGN is completely obscured in the face-on view.
Bertin Emmanuel
Cattaneo Andrea
Colombi Stephane
Combes François
Melchior Anne-Laure
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