Plasma accreted onto the surface of a neutron star can ignite due to unstable thermonuclear
burning and produce a bright flash of X-ray emission called a Type-I X-ray burst. Such …

We report new radio observations of a sample of 36 neutron star (NS) X-ray binaries, more
than doubling the sample in the literature observed at current-day sensitivities. These …

For decades cataclysmic variables (CVs) were thought to be one of the few classes of
accreting compact objects to not launch jets, and have consequently been used to constrain …

ABSTRACT Strongly magnetized (B≥ 1012 G) accreting neutron stars (NSs) are prime
targets for studying the launching of jets by objects with a solid surface; while classical jet …

Relativistic jets are observed throughout the Universe and strongly affect their surrounding
environments on a range of physical scales, from Galactic binary systems to galaxies and …

The accretion flow/jet correlation in neutron star (NS) low-mass X-ray binaries (LMXBs) is far
less understood when compared to black hole (BH) LMXBs. In this paper we will present the …

We present coordinated Chandra X-ray Observatory and Karl G. Jansky Very Large Array
observations of the transitional millisecond pulsar PSR J1023+ 0038 in its low-luminosity …

Accreting neutron stars in low-mass X-ray binaries show outflows—and sometimes jets—in
the general manner of accreting black holes. However, the quantitative link between the …

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 …

ABSTRACT Centaurus X–4 (Cen X–4) is a relatively nearby neutron star low-mass X-ray
binary that showed outbursts in 1969 and 1979, but has not shown a full outburst since. Due …