scispace - formally typeset
Open AccessJournal ArticleDOI

Angle-dependent Compton reflection of X-rays and gamma-rays

About
This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1995-04-01 and is currently open access. It has received 1538 citations till now. The article focuses on the topics: Compton scattering & Gamma ray.

read more

Content maybe subject to copyright    Report

Citations
More filters
Journal ArticleDOI

A Unified, Merger-driven Model of the Origin of Starbursts, Quasars, the Cosmic X-Ray Background, Supermassive Black Holes, and Galaxy Spheroids

TL;DR: In this article, an evolutionary model for starbursts, quasars, and spheroidal galaxies is presented, in which mergers between gas-rich galaxies drive nuclear inflows of gas, producing starburst and feeding the buried growth of supermassive black holes (BHs) until feedback expels gas and renders a briefly visible optical quasar.
Journal ArticleDOI

THE NUCLEAR SPECTROSCOPIC TELESCOPE ARRAY (NuSTAR) HIGH-ENERGY X-RAY MISSION

Fiona A. Harrison, +84 more
TL;DR: The Nuclear Spectroscopic Telescope Array (NuSTAR) as discussed by the authors is the first focusing high-energy X-ray telescope in orbit, which operates in the band from 3 to 79 keV.
Journal ArticleDOI

Local supermassive black holes, relics of active galactic nuclei and the X-ray background

TL;DR: In this paper, the authors quantify the importance of mass accretion during AGN phases in the growth of supermassive black holes (BH) by comparing the mass function of black holes in the local universe with that expected from AGN relics, which are black holes grown entirely with mass accumulation during AGNs phases.
Journal ArticleDOI

Cosmological evolution of the hard X-ray active galactic nucleus luminosity function and the origin of the hard X-ray background

TL;DR: In this article, the cosmological evolution of the hard X-ray luminosity function (HXLF) of active galactic nuclei (AGNs) in the 2-10 keV luminosity range of 1041.5-1046.5 ergs s-1 was investigated.
Journal ArticleDOI

An Observational Determination of the Bolometric Quasar Luminosity Function

TL;DR: In this paper, the authors combine a large set of quasar luminosity function (QLF) measurements from the rest-frame optical, soft and hard X-ray, and near and mid-IR bands to determine the bolometric QLF in the redshift interval z = 0-6.
Related Papers (5)