Jets from X-ray binaries

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Nomenclature: NS classes Atoll sources Z sources HB . m IS ?? ?? . m NB LB UB FB ~0.01 ~0.1 ’Hard’ atoll sources ’Soft’ atoll sources Luminosity / Eddington ’Z’ sources van der Klis 2006 Migliari & Fender 2006
XTE J1701-462: the Rosetta Stone Atoll Z-Sco Z-Cyg Homan et al. 2010
Page 1 and 2: Jets from X-ray binaries Simone Mig
Page 3 and 4: “Jets are possibly the most spect
Page 5 and 6: Stirling et al 2001 1 arcmin (2 lig
Page 7 and 8: powerful
Page 9 and 10: AGN X-ray binaries WD binaries YSOs
Page 11 and 12: Meier et al. 2001
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 47: X-ray binary population Radio detec
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 and 64: Role of the NS magnetic field?
Page 65 and 66: X-ray pulsars B> 10 12 G L 8.5 GHz
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

Jets from X-ray binaries

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