Jets from X-ray binaries
Jets from X-ray binaries Jets from X-ray binaries
X-ray pulsars B> 10 12 G L 8.5 GHz (x10 26 erg/s) 10 100 1000 10 4 NO quantitative proof yet 0.01 0.1 1 10 100 1000 L 2!10 keV (x10 36 erg/s) Migliari 2010
X-ray pulsars B> 10 12 G L 8.5 GHz (x10 26 erg/s) 10 100 1000 10 4 NO quantitative proof yet 0.01 0.1 1 10 100 1000 L 2!10 keV (x10 36 erg/s) Migliari 2010
- Page 13 and 14: M87: 1 yr Walker et al.
- Page 15 and 16: outburst: accretion disc variabilit
- Page 17 and 18: BH X-ray binaries
- Page 19 and 20: Two types of jets transient compact
- Page 21 and 22: X-ray Intensity few 100s accretion
- Page 23 and 24: X-ray Intensity few 100s accretion
- Page 25 and 26: X-ray Intensity few 100s Migliari e
- Page 27 and 28: X-ray Intensity few 100s few months
- Page 29 and 30: Miller-Jones et al.: JACPOT collabo
- Page 31 and 32: transient compact Miller-Jones et a
- Page 33 and 34: proposed Unified Scenario Fender et
- Page 35 and 36: proposed Unified Scenario Fender et
- Page 37 and 38: stellar-mass/super-massive BH conne
- Page 39 and 40: Which parameters are involved in je
- Page 41 and 42: X-ray binary population sample: 264
- Page 43 and 44: X-ray binary population sample: 264
- Page 45 and 46: X-ray binary population sample: 264
- Page 47 and 48: X-ray binary population Radio detec
- Page 49 and 50: XTE J1701-462: the Rosetta Stone At
- Page 51 and 52: Z-Cyg GX5-1 4U1701-462 CygX-2 CygX-
- Page 53 and 54: Atoll-H-S transitions Miller-Jones
- Page 55 and 56: Atoll-GX quenching at ~10% Eddingto
- Page 57 and 58: Atolls Z-Cyg Detection: all X-ray s
- Page 59 and 60: Z GX17+2 Migliari et al. 2007 GX17+
- Page 61 and 62: Z-Cyg Z-Sco X-ray intensity Atoll-G
- Page 63: Role of the NS magnetic field?
- Page 67 and 68: Role of the NS Spin?
- Page 69 and 70: Role of the NS Spin?
- Page 71 and 72: Models for jets in NSs: what are we
X-<strong>ray</strong> pulsars<br />
B> 10 12 G<br />
L 8.5 GHz<br />
(x10 26 erg/s)<br />
10 100 1000 10 4<br />
NO quantitative proof yet<br />
0.01 0.1 1 10 100 1000<br />
L 2!10 keV<br />
(x10 36 erg/s)<br />
Migliari 2010
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