The mass density in black holes inferred from the X-ray background
- 21 February 1999
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 303 (2)
- https://doi.org/10.1046/j.1365-8711.1999.02404.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 13 references indexed in Scilit:
- The Spectrum of the Extragalactic Far‐Infrared Background from theCOBEFIRAS ObservationsThe Astrophysical Journal, 1998
- TheCOBEDiffuse Infrared Background Experiment Search for the Cosmic Infrared Background. I. Limits and DetectionsThe Astrophysical Journal, 1998
- High-redshift galaxies, their active nuclei and central black holesMonthly Notices of the Royal Astronomical Society, 1998
- The Cosmic Baryon BudgetThe Astrophysical Journal, 1998
- Do nuclear starbursts obscure the X-ray background?Monthly Notices of the Royal Astronomical Society, 1998
- The cosmological evolution of the QSO luminosity density and of the star formation rateMonthly Notices of the Royal Astronomical Society, 1998
- Pair-dominated active galactic nuclei and the origin of the X-ray backgroundMonthly Notices of the Royal Astronomical Society, 1995
- Atlas of quasar energy distributionsThe Astrophysical Journal Supplement Series, 1994
- The unified Seyfert scheme and the origin of the cosmic X-ray backgroundMonthly Notices of the Royal Astronomical Society, 1994
- Remnants of the quasarsMonthly Notices of the Royal Astronomical Society, 1992