A <i>NuSTAR</i> view of SS433
Federico A. Fogantini, Federico García, J. A. Combi, S. Chaty, J. Martı́, Pedro L. Luque‐Escamilla
Abstract
Context. SS433 is a Galactic microquasar with powerful outflows (double jet, accretion disk and winds) with a well-known orbital, precessional, and nutational period. Aims. In this work we characterise different outflow parameters throughout the precessional cycle of the system. Methods. We analysed ten NuSTAR (3–70 keV) observations of ∼30 ks that span ∼1.5 precessional cycles. We extracted averaged spectra and modelled them using a combination of a double thermal jet model ( bjet ) and pure neutral and relativistic reflection ( xillverCp and relxilllpCp ) over an accretion disk. Results. We find an average jet bulk velocity of β = v / c ∼ 0.29 with an opening angle of ≲6 deg. Eastern jet kinetic power ranges from 1 to 10 39 erg s −1 , with base ‘coronal’ temperatures T o ranging from between 14 and 18 keV. Nickel-to-iron abundances remain constant at ∼9 (within 1 σ ). The western to eastern jet-flux ratio becomes ∼1 on intermediate phases, which is about 35% of the total precessional orbit. The 3–70 keV total unabsorbed luminosity of the jet and disk ranges from 2 to 20 × 10 37 erg s −1 , with the disk reflection component mainly contributing to the hard 20–30 keV excess and the stationary 6.7 keV ionised Fe line complex. Conclusions. At low opening angles Θ, we find that the jet expands sideways following an adiabatic expansion of a gas with temperature T o . Finally, the central source and lower parts of the jet could be hidden by an optically thick region of τ > 0.1 and size R ∼ N H / n e0 ∼ 1.5 × 10 9 cm ∼ 1700 r g for M BH = 3 M ⊙ .