Hostname: page-component-78c5997874-t5tsf Total loading time: 0 Render date: 2024-11-02T20:47:24.843Z Has data issue: false hasContentIssue false
  • English
  • Français

A nuclear Luminosity Function for Seyferts

Published online by Cambridge University Press:  25 May 2016

E.J.A. Meurs
E.J.A. Meurs*
Affiliation:
Dunsink Observatory Castleknock, Dublin 15, Ireland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Relations between various classes of AGN should show up when examining their LFs. For Seyfert galaxies, such studies have been affected by the prevalence of (essentially) integrated magnitudes. Proper nuclear magnitudes have been determined in an effort of CCD imaging, which enable an appropriate comparison with QSOs.

Type
Cosmological Implications
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 541 - 542
Copyright
Copyright © Kluwer 1996 

References

Meurs, E.J.A. (1986) in The optimization of the use of CCD detectors in astronomy , Baluteau, & D'Odorico, (Eds), p. 105 Google Scholar
Meurs, E.J.A. and Wilson, A.S. (1984) A&A 136, 206 Google Scholar
Meurs, E.J.A., Bonifacio, V. and Lima, N. (1991) 3rd ESO/ST-ECF Data Analysis Workshop , Grosbol, & Warmels, (Eds), p. 45 Google Scholar