Multi-wavelength observations of compact jets in a neutron star X-ray binary

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Scientific paper

Our cycle-2 Spitzer IRAC observations revealed the first spectral evidence for compact jets in low-luminosity neutron star (NS) X-ray binary, and furthermore, the optically thin (`break') part of its synchrotron spectrum in 4U~0614+091. As a follow-up of this major result, we ask for simultaneous IRAC and VLA observations of 4U~0614+091 together with quasi-simultaneous MIPS observations at 24um. These multi-wavelength coverage, will give us the first complete broadband spectrum of a compact jet in a low-luminosity NS system. Low-luminosity NSs are important especially because they are the best candidate for a direct comparison of the disc/jet properties in BHs. We will measure observable jet parameters never measured before together in a NS system (e.g. the spectral index in the optically thick and optically thin part of the spectrum, and the break frequency), we will have a precise estimate of the power in the jet and, together with available simultaneous X-rays observations, we will assess the efficiency of the jet production, estimating the fraction of the accreted power that is channeled into the jet.

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