Dark jets in the soft X-ray state of black hole binaries?

S. Drappeau (1) , J. Malzac (1) , M. Coriat (1) , J. Rodriguez (2) , T.M. Belloni , R. Belmont (1, 2) , M. Clavel (2) , S. Chakravorty (3) , S. Corbel (2) , J. Ferreira (3) , P. Gandhi , G. Henri (3) , P. -O. Petrucci (3)

1 IRAP - Institut de recherche en astrophysique et planétologie
2 AIM (UMR7158 / UMR_E_9005 / UM_112) - Astrophysique Interprétation Modélisation
3 IPAG - Institut de Planétologie et d'Astrophysique de Grenoble

X-ray binary observations led to the interpretation that powerful compact jets, produced in the hard state, are quenched when the source transitions to its soft state. The aim of this paper is to discuss the possibility that a powerful dark jet is still present in the soft state. Using the black hole X-ray binaries GX339–4 and H1743–322 as test cases, we feed observed X-ray power density spectra in the soft state of these two sources to an internal shock jet model. Remarkably, the predicted radio emission is consistent with current upper limits. Our results show that for these two sources, a compact dark jet could persist in the soft state with no major modification of its kinetic power compared to the hard state.

Mots clés: accretion; accretion discs; black hole physics; radiation mechanisms: non-thermal; relativistic processes; shock waves; X-rays: binaries

Domaines: Astrophysique [astro-ph]

S. Drappeau, J. Malzac, M. Coriat, J. Rodriguez, T.M. Belloni, et al.. Dark jets in the soft X-ray state of black hole binaries?. Monthly Notices of the Royal Astronomical Society, 2017, 466 (4), pp.4272-4278. ⟨10.1093/mnras/stw3277⟩. ⟨hal-01554842⟩