Abstract
The likely merger process and the properties of the stellar populations in the I Zw 1 host galaxy are analyzed on the basis of multi-wavelength observations4 and N-body simulations. The data give a consistent picture of I Zw 1, with properties between those of ultra-luminous infrared galaxies (ULIRGs) and QSOs as displayed by transition objects in the evolutionary sequence of active galaxies.
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© 1997 Springer-Verlag Berlin Heidelberg
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Scharwächter, J. et al. (1997). The Nearby QSO Host I Zw 1: NIR Probing of Structural Properties and Stellar Populations. In: Pfalzner, S., Kramer, C., Straubmeier, C., Heithausen, A. (eds) The Dense Interstellar Medium in Galaxies. Springer Proceedings in Physics, vol 91. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-18902-9_24
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DOI: https://doi.org/10.1007/978-3-642-18902-9_24
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