Multi-Resonance Orbital Model of High-Frequency Quasi-Periodic Oscillations: Possible High-Precision Determination of Black Hole and Neutron Star Spin
Astronomy and Astrophysics - France
doi 10.1051/0004-6361/201219724
Full Text
Open PDFAbstract
Available in full text
Date
March 14, 2013
Authors
Publisher
EDP Sciences