Résumé
Inspiraling
and merging compact binaries consisting of neutron stars (NS) and black
holes (BH) are strong sources of gravitational waves, and are expected
to give rise to frequent signals in future groundbased detectors. 
Bibliographie
 M. Maggiore, Gravitational Waves (Volume 1), section 4.1 / section 7.17.4 and 7.7
 (for fun) http://www.blackholehunter.org/index_fr.html
 B.S.
Sathyaprakash, B.F. Schutz., 'Physics, Astrophysics and Cosmology with
Gravitational Waves', Living Rev. Relativity 12, (2009), 2 [http://arxiv.org/abs/arXiv:0903.0338], sections 5, 4.5, 4.8
 S. Babak et al., 'Searching for gravitational waves from binary coalescence', Phys.Rev. D87 (2013) 024033 [http://arxiv.org/abs/arXiv:1208.3491]
 B. Allen et al., 'FINDCHIRP', Phys.Rev. D85 (2012) 122006 [http://arxiv.org/abs/grqc/0509116]
