How X-ray Experiments See Black Holes: Past, Present and Future


Click here to start

Table of contents

How X-ray Experiments See Black Holes: Past, Present and Future

Introduction

Accretion Review

Mass Determination

Mass Determination

PowerPoint Presentation

Disk Jet Interaction

Old Faithful Black Hole/GRS 1915+105

Quasi-Periodic Oscillation

Relativistic Effects : frame-dragging

Spin Determination

Flare from our Galactic Center

Spectral Line Analysis

Chandra:3C273 Jet

Chandra: M82 Starburst Galaxy

The Constellation X-ray Mission

BH Mass and Spin using Iron K Line

Black Hole Evolution

MAXIM: MicroArcsecond X-ray Imaging Mission

Summary

For more information:

Author: Lynn Cominsky

E-mail: lynnc@charmian.sonoma.edu

Homepage: http://www-glast.sonoma.edu/~lynnc