2021MNRAS.508L...6R

The persistently bright ultracompact neutron star low-mass X-ray binary 4U 1820-30 displays an ∼170 d accretion cycle, evolving between phases of high and low X-ray modes, where the 3-10 keV X-ray flux changes by a factor of up to ≃8. The source is generally in a soft X-ray spectral state, but may transition to a harder state in the low X-ray mode. Here, we present new and archival radio observations of 4U 1820-30 during its high and low X-ray modes. For radio observations taken within a low mode, we observed a flat radio spectrum consistent with 4U 1820-30 launching a compact radio jet. However, during the high X-ray modes the compact jet was quenched and the radio spectrum was steep, consistent with optically thin synchrotron emission. The jet emission appeared to transition at an X-ray luminosity of L_X (3-10 keV)_ ∼3.5 ×10³⁷ (D/ 7.6 kpc)² erg s^–1. We also find that the low-state radio spectrum appeared consistent regardless of X-ray hardness, implying a connection between jet quenching and mass accretion rate in 4U 1820-30, possibly related to the properties of the inner accretion disc or boundary layer.