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Waldek was interested in this subject during the 2002/2003 academic year. Any students interested in this theme, please edit this page a translate this to a page FormacjiGalAGN w po polsku.


  • FLRW model

  • zjednoczony AGN model

galaktyka (formatowanie modelu)

  • mała gęstość perturbacji o 10^{-5} w z=1100 rosnącym w czasie
przez grawitacyjne rozpadanie się i formowanie ciemnej materii,(baryonic + non-baryonic) aureoli, które łączą się i stają się większe.

  • chłodne gazy i formy gwiazd w aureolach



SMBH/AGN formation questions

  • Do any SMBHs start forming before DM haloes have formed?
  • Do SMBHs form in the "initial" collapse of a halo, or only when haloes and/or galaxies merge?
  • Do SMBHs "light up" as AGNs during major mergers of galaxies (mergers between two galaxies of similar mass) or also during minor
mergers (galaxies of different mass, e.g. ratio 10:1)?

intuition/education - nice g formation movies

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Topic revision: r4 - 01 Feb 2007, AniaKozlowska
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