What is the maximun IR luminosity of a single spiral galaxy?

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Scientific paper

A new sample of IRAS galaxies at high galactic latitudes is made by optical identifications of IRAS point sources. In many cases several galaxies or groups of galaxies are the optical counterparts of IR sources. To distinguish the exact objects responsible for the IR radiation, cross-correlations with radio catalogs (particularly NVSS) have been made. Really, in most of the mentioned cases, only one of the components coincides with radio coordinates. Most of these objects are AGNs according to spectral observations with OHP 1.93m, Byurakan 2.6m and SAO 6m telescopes. Presence of starburst and AGN phenomena, as well as interactions allows to study the origin and mutual influence of star-formation and activity processes on each other.

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