Academic Journal

Dust obscured star formation and AGN fueling in hierarchical models of galaxy evolution

التفاصيل البيبلوغرافية
العنوان: Dust obscured star formation and AGN fueling in hierarchical models of galaxy evolution
المؤلفون: A. W. Blain, Allon Jameson, Ian Smail, M. S. Longair, J. -p. Kneib, R. J. Ivison
المساهمون: The Pennsylvania State University CiteSeerX Archives
المصدر: http://arxiv.org/pdf/astro-ph/9906311v1.pdf.
سنة النشر: 2008
المجموعة: CiteSeerX
الوصف: A large fraction of the luminous distant submillimetre-wave galaxies recently detected using the Submillimetre Common-User Bolometer Array (SCUBA) camera on the James Clerk Maxwell Telescope appear to be associated with interacting optical counterparts. We investigate the nature of these systems using a simple hierarchical clustering model of galaxy evolution, in which the large luminosity of the SCUBA galaxies is assumed to be generated at the epoch of galaxy mergers in a burst of either star formation activity or the fueling of an active galactic nucleus (AGN). The models are well constrained by the observed spectrum of the far-infrared/submillimetre-wave background radiation and the 60-µm counts of low-redshift IRAS galaxies. The ratio between the total amount of energy released during a merger and the mass of dark matter involved must increase sharply with redshift z at z < ∼ 1, and then decrease at greater redshifts. This result is independent of the fraction of the luminosity of mergers that is produced by starbursts and AGN. One additional parameter – the
نوع الوثيقة: text
وصف الملف: application/pdf
اللغة: English
Relation: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.9642; http://arxiv.org/pdf/astro-ph/9906311v1.pdf
الاتاحة: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.256.9642
http://arxiv.org/pdf/astro-ph/9906311v1.pdf
Rights: Metadata may be used without restrictions as long as the oai identifier remains attached to it.
رقم الانضمام: edsbas.9AE7B431
قاعدة البيانات: BASE