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L. E. Simon, F. W. Hamann and M. Pettini, “Physical Properties of Absorbers in High Redshift Quasars,” In: R. Guzmán, C. Packham, J. M. Rodríguez-Espinosa and S. Torres-Peimbert, Eds., First Light Science with the GTC, Instituto de Astronomaia, Universidad Nacional Autao- noma de Maexico, Miami, Vol. 29, 2007, p. 177.

has been cited by the following article:

• TITLE: Pending Problems in QSOs

  AUTHORS: Martín López-Corredoira

  KEYWORDS: Quasars, General-Cosmology, Miscellaneous

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.1 No.2, June 29, 2011

  ABSTRACT: Quasars (Quasi Stellar Objects, abbreviated as QSOs) are still nowadays, close to half a century after their discovery, objects which are not completely understood. In this brief review a description of the pending problems, inconsistencies and caveats in the QSO's research is presented. The standard paradigm model based on the existence of very massive black holes that are responsible for the QSO's huge luminosities, re-sulting from to their cosmological redshifts, leaves many facts without explanation. There are several obser-vations which lack a clear explanation, for instance: the absence of bright QSOs at low redshifts, a mysteri-ous evolution not properly understood; the inconsistencies of the absorption lines, such as the different structure of the clouds along the QSO's line of sight and their tangential directions; the spatial correlation between QSOs and galaxies; and many others.