Jets from X-ray binaries
Jets from X-ray binaries Jets from X-ray binaries
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08.06.2015
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NS X-ray binaries
Which parameters are involved in jet formation? ⋅ M Spin Magn. field
- 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: stellar-mass/super-massive BH conne
- 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 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
Which<br />
parameters<br />
are involved in<br />
jet formation?<br />
⋅<br />
M<br />
Spin<br />
Magn. field
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