Jet-accretion coupling in low/hard state Galactic black hole candidates

2004 ◽  
Vol 132 ◽  
pp. 363-368 ◽  
Author(s):  
E. Gallo ◽  
R.P. Fender ◽  
G.G. Pooley
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 ◽  
...  

1992 ◽  
Author(s):  
Wm. A. Wheaton ◽  
James C. Ling ◽  
R. T. Skelton ◽  
Alan Harmon ◽  
Gerald J. Fishman ◽  
...  

2010 ◽  
Vol 404 (1) ◽  
pp. L94-L98 ◽  
Author(s):  
T. Muñoz-Darias ◽  
S. Motta ◽  
D. Pawar ◽  
T. M. Belloni ◽  
S. Campana ◽  
...  

1998 ◽  
Vol 500 (2) ◽  
pp. 899-908 ◽  
Author(s):  
J. E. Grove ◽  
W. N. Johnson ◽  
R. A. Kroeger ◽  
K. McNaron‐Brown ◽  
J. G. Skibo ◽  
...  

Author(s):  
W. S. Paciesas ◽  
B. A. Harmon ◽  
B. C. Rubin ◽  
C. A. Wilson ◽  
S. N. Zhang

2012 ◽  
Vol 8 (S290) ◽  
pp. 249-250
Author(s):  
Y. J. Lei ◽  
H. T. Zhang ◽  
A. L. Luo ◽  
Y. H. Zhao

AbstractWe study the cross-correlation between X-rays of different energies for the atoll-type source 4U 1608–52 with RXTE, and find the cross-correlation evolutes along the different branches. The anti-correlation is reported from the Galactic black hole candidates and Z-type luminous sources in their hard states. Our results are a little different from the Z-type sources. Here we provide the first evidence that a similar anti-correlated feature can also be found in atoll-type source, and it is not corresponding to the lowest accretion rate.


Sign in / Sign up

Export Citation Format

Share Document