No CrossRef data available.
Article contents
Low-Ionization Balqsos: Warm Ultraluminous Galaxies at High Redshifts
Published online by Cambridge University Press: 25 May 2016
Extract
A decade ago Sanders et al. (1988a, b) proposed a possible QSO formation scenario as a sequence of Galaxy Mergers → Ultraluminous IR Galaxies (ULIRGs) → Warm ULIRGs → QSOs. Since then, this proposal has become a paradigm against which all the subsequent observations will be compared. Fortunately for us, this paradigm makes two specific predictions: that is, 1) ULIRGs are powered by hidden AGNs, and 2) ULIRGs should be more abundant at z ~ 2, where the comoving density of optically-selected QSOs is sharply peaking up.
- Type
- Deep Fields & Evolution
- Information
- Symposium - International Astronomical Union , Volume 186: Galaxy Interactions at High and Low Redshift , 1999 , pp. 475 - 478
- Copyright
- Copyright © Kluwer 1999