outbursts and state transitions in black hole candidates observed by maxi hitoshi negoro (nihon u.)...
TRANSCRIPT
Outbursts and
State Transitions in
Black Hole Candidates observed by MAXI
Hitoshi Negoro (Nihon U.)& MAXI Team
Outline
• Black Hole Transients/Transient Events observed with MAXI
• Discovery of a new black-hole candidate MAXI J1659-152
• Comparison with..– XTE J1752-223– Soft state transitions in Cyg X-1 and GX 339-4
• Some comments on other BHCs• What triggers the state transition ?• Summary
Black Hole Candidates
XTE J1752-223 (#2259, 2378*, 2396)
GX 339-4 (#2380)
H1743-322 (#2364, 2378, 2774)
4U 1630-47 (#2363)Cyg X-1 (#2711)
GRS 1915+105
Swift J1753.5-0127(#2341)
LMC X-1, X-3
ATel # in Red : Possible State Transition
MAXI J1659-152 (#2873)
Swift/BAT triggered(Mangano+ GCN 11296)as GRB 20100928A
Discovery of MAXI J1659-152
MAXI/GSC triggered(Negoro+ ATel 2783)
Nova AlertSystem: Ozawa+ Suwa+
(MAX
I 2 -
20 k
eV)
Color-Intensity Diagram MAXI J1659-152
SoftState Hard
State
“Stable” Intermediate (very high?) State
2-20
keV
Flu
x
Color-Intensity DiagramComparison with XTE J1752-223
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“stable” 2nd hardstate ?
Nakahira+ 2010, also see Poster
SoftState
Cyg X-1 and GX 339-4 both in the soft state ?
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Cyg X-1
GX 339-4
Color-Intensity Diagram GX 339-4
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Finder+ 04
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SSC 1 yr Image (Kimura+)
Negoro+ ATel 2341
Nature of the Soft Excess Component
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Miller+ 2006
Hiemstra+ 2008 Durant+ 2008
Short-term ?
~ days ?
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XTE J1752-223 MAXI J1659-152
GX 339-4 Cyg X-1
Dark and Fast Transition
Soft-State Source or Intermediate-State Source ?cf. Gierlinski & Newton 2006
Bright and Slow Transition
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Discussion
Yu+ 2007
Yu et al. found a positive correlation between the peak luminosities of the hard state and those of the soft state.
Discussion
Color
Inte
nsit
yThe soft state transition The soft state transition is not directly associated is not directly associated with an absolute m-dot with an absolute m-dot value (?). This suggests value (?). This suggests
magnetic force plays magnetic force plays some important role.some important role.
The disk is still supportedThe disk is still supported magnetically ?magnetically ?
Oda+ (2009) explained two types of soft-state transitionsby a magnetically supported disk model.
Summary• MAXI observed X-ray outbursts from H1743-322, 4U 16
30-472, GX 339-4, XTE J1752-223, and MAXI J1659-152.
• MAXI also observed many state transitions including transitions in Swift J1753.5-0127 and Cyg X-1.
• Color-Intensity diagrams of these sources show two types of transitions to the soft (and intermediate) state.– Cyg X-1 and MAXI J1659-152 are stable in the intermediate (ve
ry high) state. – GX 339-4 and XTE J1752-223 are stable in the soft state.
• The magnetically supported disk model is favorable to the observed features of the intermediate state.
• The following futures are, however, still open questions.– luminosity dependence– Regularity– Environment(?) dependence (difference in initial magnetic force)
Neutron Star Studies
NGC 6440 (#2360)
ATel # in Red : Possible State Transition
A0535+26 (#2277)
4U 1608-52 (#2462)
Cir X-1 (#2608, 2674)4U 2206+54 (#2271)
4U 1711 (#2425)
V 0332+53(#2369, 2427)
LMC X-4
GX 304-1 (#2297)
4U 1323+619(#2399)
Cyg X-3 (#2404, 2635)
LS V +44 17(#2527)
4U 1954+319(#2702)
XTE J1709-267 (#2425)
ATel # in Yellow : Burst or Flare
Black Hole Studies
XTE J1752-223 (#2259, 2378*, 2396)
GX 339-4 (#2380)
H1743-322 (#2364, 2378)
4U 1630-47 (#2363)Cyg X-1 (#2711)
GRS 1915+105
Swift J1753.5-0127(#2341)
LMC X-1, X-3
ATel # in Red : Possible State Transition
PCA ATCA
PCA MAXI
Swift+MAXI PCA MAXI