Abstract
1	Introduction
2	Accretion Induced Collapse
	2.1	Collapse scenario
	2.2	Formation rate
	2.3	GW emission mechanisms
	2.4	Numerical predictions of ...
	2.5	Going further
3	Collapse of Massive Stars
	3.1	Collapse scenario
	3.2	Formation rate
	3.3	GW emission mechanisms
	3.4	Numerical predictions of ...
	3.5	Going further
4	Collapse of Population III Stars
	4.1	Collapse scenario
	4.2	Formation rate
	4.3	GW emission mechanisms
	4.4	Numerical predictions of ...
5	Collapse of Supermassive Stars
	5.1	Collapse scenario
	5.2	Formation rate
	5.3	GW emission mechanisms
	5.4	Numerical predictions of ...
6	Summary
7	Acknowledgements

References

---