scholarly journals Multiwavelength Observations of the Galactic Black Hole Transient 4U 1543−47 during Outburst Decay: State Transitions and Jet Contribution

2005 ◽  
Vol 622 (1) ◽  
pp. 508-519 ◽  
Author(s):  
E. Kalemci ◽  
J. A. Tomsick ◽  
M. M. Buxton ◽  
R. E. Rothschild ◽  
K. Pottschmidt ◽  
...  
2000 ◽  
Vol 544 (1) ◽  
pp. 443-452 ◽  
Author(s):  
A. R. Rao ◽  
J. S. Yadav ◽  
B. Paul

2004 ◽  
Vol 603 (1) ◽  
pp. 231-241 ◽  
Author(s):  
E. Kalemci ◽  
J. A. Tomsick ◽  
R. E. Rothschild ◽  
K. Pottschmidt ◽  
P. Kaaret

2006 ◽  
Vol 639 (1) ◽  
pp. 340-347 ◽  
Author(s):  
E. Kalemci ◽  
J. A. Tomsick ◽  
R. E. Rothschild ◽  
K. Pottschmidt ◽  
S. Corbel ◽  
...  

Author(s):  
Satoshi Nakahira ◽  
Megumi Shidatsu ◽  
Kazuo Makishima ◽  
Yoshihiro Ueda ◽  
Kazutaka Yamaoka ◽  
...  

2021 ◽  
Vol 502 (1) ◽  
pp. L72-L78
Author(s):  
K Mohamed ◽  
E Sonbas ◽  
K S Dhuga ◽  
E Göğüş ◽  
A Tuncer ◽  
...  

ABSTRACT Similar to black hole X-ray binary transients, hysteresis-like state transitions are also seen in some neutron-star X-ray binaries. Using a method based on wavelets and light curves constructed from archival Rossi X-ray Timing Explorer observations, we extract a minimal timescale over the complete range of transitions for 4U 1608-52 during the 2002 and 2007 outbursts and the 1999 and 2000 outbursts for Aql X-1. We present evidence for a strong positive correlation between this minimal timescale and a similar timescale extracted from the corresponding power spectra of these sources.


1998 ◽  
Vol 184 ◽  
pp. 65-66
Author(s):  
Marc Freitag ◽  
Willy Benz

Massive but invisible black holes (BH) are often assumed to lurk in the center of many galaxies but definitive proof of their existence has not yet been established. However, in the surrounding stellar cluster stars are unavoidably being destroyed by tidal disruptions and stellar collisions liberating of order 1M⊙ in each event. The subsequent accretion of this gas by the BH could bring it back to “life” and reveal its presence.


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.


2002 ◽  
pp. 2279-2288 ◽  
Author(s):  
SANDIP K. CHAKRABARTI ◽  
S.G. MANICKAM ◽  
A. NANDI ◽  
A.R. RAO

2003 ◽  
Vol 403 (1) ◽  
pp. L15-L18 ◽  
Author(s):  
P. Reig ◽  
N. D. Kylafis ◽  
D. Giannios

2015 ◽  
Vol 67 (1) ◽  
pp. 11-11 ◽  
Author(s):  
A. Yoshikawa ◽  
S. Yamada ◽  
S. Nakahira ◽  
M. Matsuoka ◽  
H. Negoro ◽  
...  

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