On the mass determination of collapsed objects in close binaries: Applications to black-holes and neutron stars

1974 ◽  
Vol 27 (2) ◽  
pp. 293-301 ◽  
Author(s):  
Yoji Kondo
2017 ◽  
Vol 2 (1) ◽  
pp. 63-68 ◽  
Author(s):  
J. E. Mejía-Restrepo ◽  
P. Lira ◽  
H. Netzer ◽  
B. Trakhtenbrot ◽  
D. M. Capellupo

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

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

2008 ◽  
Vol 7 (1) ◽  
pp. 64-70
Author(s):  
Kenath Arun

This paper shall look into the systems of compact astrophysical objects (black holes, neutron stars and white dwarfs) concerning mainly with binary systems. Determination of the orbital periods, velocities, etc, for such systems and also, the energy lost from the system through gravitational waves has been made, From the concept of energy loss, the merger of the two black holes in the system has been considered and the typical time required for the merger is calculated.


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

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