OUTLINE X-RAY STATES & RADIO JETS (BLACK HOLES) Radio phenomenology vs accretion modes LUMINOSITY CORRELATIONS (BLACK HOLES) radio/X-ray NIR/X-ray dependence on X-ray binary parameters (lack thereof) Update: clustering algorithms, Bayesian analysis, linear regression BLACK HOLES VS NEUTRON STARS radio luminosity, bulk velocity BLACK HOLE SPIN & JET POWER

cf. Sera Markoff

Cyg X-1 Stirling et al.‘01 GRS Mirabel et al. ‘94 1E Mirabel et al. al ‘99 SS433 Blundell et al. 2004

Meyer, Liu & Meyer-Hofmeister 2006 Radiatively inefficient inflow (ADAF, CDAF, JDAF, ADIOS..) McClintock & Remillard 2006

Meyer, Liu & Meyer-Hofmeister 2006 McClintock & Remillard 2006 Cyg X-1 Stirling et al.‘01 Radiatively inefficient inflow (ADAF, CDAF, JDAF, ADIOS..)

X-ray states: high/soft (thermal dominat) Radiatively efficient inflow (thin disc) McClintock & Remillard 2006 Meyer, Liu & Meyer-Hofmeister 2006

X-ray states: high/soft (thermal dominat) Radiatively efficient inflow (thin disc) SUPPRESSED McClintock & Remillard 2006 Meyer, Liu & Meyer-Hofmeister 2006

X-ray states: hard to soft transition McClintock & Remillard 2006 JETS DURING HARD-TO-SOFT TRANSITIONS GRS Mirabel et al 1994 Meyer, Liu & Meyer-Hofmeister 2006

Fender Belloni Gallo 2004; Fender Homan Belloni 2009

Corbel et al U Angelini et al Corbel et al. 2005

Gallo et al Jet-powered nebulae Cygnus X-1, Isaac Newton Russell et al SS433 W50, VLA, Dubner et al Cyg X-1, WRST

Luminosity correlations I. X-ray/radio Corbel et al 2003, Gallo et al 2003, Gallo 2007

Luminosity correlations II. NIR/radio Russell et al 2006

Soleri & Fender 2010 Roche lobe radius Orbital period (No) Orbital parameters dependence

Soleri & Fender 2010 (Weak) Inclination dependence (NIR/X-ray)

Coriat et al Tracks & Accretion mode transition ?

Gallo et al. in prep. Black hole X-ray binaries in the radio/X-ray domain: a statistical approach

Gallo et al. in prep. Black hole X-ray binaries in the radio/X-ray domain: a statistical approach

Gallo et al. in prep. Black hole X-ray binaries in the radio/X-ray domain: a statistical approach

Gallo et al. in prep. Black hole X-ray binaries in the radio/X-ray domain: a statistical approach

Black Holes vs Neutron Stars I. Black points: BHs Red points: NS atoll sources Blue points: NS Z sources after Migliari & Fender 2006

Black Holes vs Neutron Stars II. Fender et al 2004

Cyg X-1 Stirling et al.‘01 GRS Mirabel et al. ‘94 1E Mirabel et al. al ‘99 SS433 Blundell et al Fabian et al 2000 obs / em

Cyg X-1 Stirling et al.‘01 Cf. Miller, Fabian, Cackett, Miniutti, Reis, Reynolds et al.

Cyg X-1 Stirling et al.‘01 R ISCO  a * H (Kubota et al 2004) T eff 4..after color correction (cf. S. Davis) cf. McClintock, Shafee, Narayan, Steiner, Gou, Liu, Done, Gierlinski, Middleton

Constraints on spin powering of jets Fender Gallo Russell 2010

Hard state: Steady jets ReflectionDisk Fender Gallo Russell 2010 No apparent jet/spin correlation

State transitions: Transient jets ReflectionDisk Fender Gallo Russell 2010 No apparent jet/spin correlation

X-RAY STATES & RADIO JETS (BLACK HOLES) Phenomenology – well understood. LUMINOSITY CORRELATIONS (BLACK HOLES) No dependence on X-ray binary orbital parameters, nor outburst properties. Very weak dependence on jet axis. Statistically significant evidence for 2 separate clusters in the radio/X-ray domain. Universal correlation..no longer such. BLACK HOLES VS NEUTRON STARS NSs factor ~30 fainter in radio However: the most relativistic jet source in the Galaxy is a neutron star BLACK HOLE SPIN & JET POWER No apparent relation: IF the measurements are robust (..) => Jets are not powered by BH rotational energy SUMMARY