Evolution of massive close binaries and formation of neutron stars and black holes

1976 ◽  
Vol 40 (1) ◽  
pp. 115-133 ◽  
Author(s):  
A. G. Massevitch ◽  
A. V. Tutukov ◽  
L. R. Yungelson
2000 ◽  
Vol 177 ◽  
pp. 579-584
Author(s):  
V. Kalogera

AbstractThe coalescence of close binary systems with two compact objects (neutron stars and black holes) are considered to be promising sources of gravitational waves for the currently built laser interferometers. Here, I review the current Galactic coalescence estimates derived both theoretically and empirically. I discuss the uncertainties involved as well as ways of obtaining an upper limit to the coalescence rate of two neutron stars.


2020 ◽  
Vol 896 (1) ◽  
pp. 56 ◽  
Author(s):  
S. E. Woosley ◽  
Tuguldur Sukhbold ◽  
H.-T. Janka

1973 ◽  
Vol 110 (7) ◽  
pp. 441 ◽  
Author(s):  
Ya.B. Zel'dovich
Keyword(s):  

1998 ◽  
Vol 11 (1) ◽  
pp. 28-41
Author(s):  
I.D. Novikov

Some 30 years ago very few scientists thought that black holes may really exist. Attention focussed on the black hole hypothesis after neutron stars had been discovered. It was rather surprising that astrophysicists immediately ‘welcomed’ black holes. They found their place not only in the remnants of supernova explosions but also in the nuclei of galaxies and quasars.


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