<--- Back to Details
First PageDocument Content
Gravitation / General relativity / Star types / Galaxies / Numerical relativity / Binary black hole / Gravitational wave / Supermassive black hole / Spin-flip / Physics / Astronomy / Black holes
Date: 2012-11-04 13:11:01
Gravitation
General relativity
Star types
Galaxies
Numerical relativity
Binary black hole
Gravitational wave
Supermassive black hole
Spin-flip
Physics
Astronomy
Black holes

Binary black hole mergers

Add to Reading List

Source URL: astro.berkeley.edu

Download Document from Source Website

File Size: 260,00 KB

Share Document on Facebook

Similar Documents

Supermassive black hole with torn-apart star (artist’s impression)

DocID: 1vbjf - View Document

A Deep Chandra Look at the Bondi Region of the Supermassive Black Hole in NGC 3115 Jimmy Irwin1,Ka-Wah Wong1, Roman Shcherbakov2, Mihoko Yukita1, Jay Strader3, Aaron Romanowsky4,5, Dacheng

DocID: 1uZ1F - View Document

LETTER Cold, clumpy accretion toward an active supermassive black hole Grant R. Tremblay1,2,† , J. B. Raymond Oonk3,4 , Franc¸oise Combes5 , Philippe Salom´e5 , Christopher O’Dea6,7 , Stefi A. Baum6,8 , G. Mark Voi

DocID: 1sNds - View Document

The Astrophysical Journal, 606:799–803, 2004 May 10 # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. CONSTRAINING THE PROPERTIES OF SUPERMASSIVE BLACK HOLE SYSTEMS USING PULSAR TIMING:

DocID: 1rOcg - View Document

Astronomy / General relativity / Gravitational-wave astronomy / Physics / Black holes / Galaxies / Gravitation / Extreme mass ratio inspiral / Gravitational wave / Evolved Laser Interferometer Space Antenna / Gravitational-wave observatory / Supermassive black hole

INSTITUTE OF PHYSICS PUBLISHING CLASSICAL AND QUANTUM GRAVITY Class. Quantum GravS1595–S1606

DocID: 1rres - View Document