scholarly journals Accretion disk onto boson stars: A way to supplant black hole candidates

2006 ◽  
Vol 73 (2) ◽  
Author(s):  
F. Siddhartha Guzmán
2007 ◽  
Vol 663 (2) ◽  
pp. 1201-1206 ◽  
Author(s):  
Gabor Pszota ◽  
Wei Cui

1998 ◽  
Vol 188 ◽  
pp. 135-138
Author(s):  
T. Dotani

Structure of the accretion disk is compared between the soft and hard states of Cyg X-1 using the ASCA data. Large uncertainty of the disk parameters in hard state prevent us from drawing clear conclusion, but the data are consistent with a factor of 3 larger (optically thick) inner disk boundary in the hard state than in the soft state.


1987 ◽  
Vol 125 ◽  
pp. 247-247
Author(s):  
R. Hoshi ◽  
H. Inoue

It is well known that black hole candidates, Cyg X-1 and GX 339-4, have distinct high and low states, known as bimodal states. Detailed spectroscopic studies of these X-ray sources have revealed high and low states corresponding to optically thick and thin states of the surrounding accretion disks.


1998 ◽  
Vol 507 (1) ◽  
pp. 131-144 ◽  
Author(s):  
Pavel B. Ivanov ◽  
Igor V. Igumenshchev ◽  
Igor D. Novikov

Nature ◽  
2019 ◽  
Vol 570 (7759) ◽  
pp. 83-86 ◽  
Author(s):  
Elena M. Murchikova ◽  
E. Sterl Phinney ◽  
Anna Pancoast ◽  
Roger D. Blandford

2007 ◽  
Vol 22 (10) ◽  
pp. 1875-1898 ◽  
Author(s):  
ORHAN DÖNMEZ

We investigate the special cases of the formation of shocks in the accretion disks around the nonrotating (Schwarzschild) black holes in cases where one or few stars perturb the disk. We model the structure of disk with a 2D fully general relativistic hydrodynamic code and investigate a variety of cases in which the stars interacting with the disk are captured at various locations. We have found the following results: (1) if the stars perturb the disk at nonsymmetric locations, a moving one-armed spiral shock wave is produced and it destroys the disk eventually; (2) if the disk is perturbed by a single star located close to the black hole, a standing shock wave is produced while the disk becomes an accretion tori; (3) if the disk is perturbed by stars at symmetric locations, moving two-armed spiral shock waves are produced while the disk reaches a steady state; (4) continuous injection of matter into the stable disk produces a standing shock wave behind the black hole. Our outcomes reinforce the view that different perturbations on the stable accretion disk carry out different types of shock waves which produce Quasi-Periodic Oscillation (QPO) phenomena in galactic black hole candidates and it is observed as a X-ray.


2001 ◽  
Vol 320 (3) ◽  
pp. 316-326 ◽  
Author(s):  
M. A. Nowak ◽  
J. Wilms ◽  
W. A. Heindl ◽  
K. Pottschmidt ◽  
J. B. Dove ◽  
...  

2002 ◽  
Vol 573 (2) ◽  
pp. 754-763 ◽  
Author(s):  
Julian H. Krolik ◽  
John F. Hawley
Keyword(s):  

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