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- W88005180 abstract "Ultraluminous IRAS Galaxies (ULG's) have luminosities comparable to quasars while their space density is much higher than that of active galaxies. Much debate has centered around the origin of the energy source for these objects, whether this is a burst of star formation or a hidden quasar. The sample studied here is the Sanders et al. (1988) sample, 10 objects with L FIR ≥ 10 12 L ⊙ . We discuss our new observations at X-ray and submm wavelengths together with other published data for some of the objects. Some useful ideas can be gained from comparisons of the shape of the spectral energy distributions (SED's) of the ultraluminous objects with other “archetype” objects such as typical starbursts i.e. M82 or type 2 AGN i.e. NGC1068." @default.
- W88005180 created "2016-06-24" @default.
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- W88005180 date "1994-01-01" @default.
- W88005180 modified "2023-09-25" @default.
- W88005180 title "Multiwavelength Energy Distributions of Ultraluminous IRAS Galaxies" @default.
- W88005180 cites W1994703407 @default.
- W88005180 doi "https://doi.org/10.1017/s0074180900175370" @default.
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