CONSTRAINING THE QUADRUPOLE MOMENT OF STELLAR-MASS BLACK HOLE CANDIDATES WITH THE CONTINUUM FITTING METHOD-Reference-Cited by-同舟云学术

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CONSTRAINING THE QUADRUPOLE MOMENT OF STELLAR-MASS BLACK HOLE CANDIDATES WITH THE CONTINUUM FITTING METHOD

Published:2011-04-01 Issue:2 Volume:731 Page:121
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Bambi Cosimo,Barausse Enrico

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/731/i=2/a=121/pdf

Reference96 articles.

1. How to Observe a Non-Kerr Spacetime Using Gravitational Waves

2. Apparent shape of super-spinning black holes

3. Accretion process onto super-spinning objects

4. Outflows from accreting super-spinars

5. Shape and position of the shadow in the δ = 2 Tomimatsu–Sato spacetime

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