Neutron stars are associated with diverse physical phenomena that take place in conditions
characterized by ultrahigh densities as well as intense gravitational, magnetic and radiation …

We study an empirical model for a unified description of the power spectra of accreting
neutron stars and black holes. This description is based on a superposition of multiple …

A new scheme for testing nuclear matter equations of state (EoSs) at high densities using
constraints from neutron star (NS) phenomenology and a flow data analysis of heavy-ion …

The optical/near-infrared (OIR) region of the spectra of low-mass X-ray binaries (XBs)
appears to lie at the intersection of a variety of different emission processes. In this paper we …

Detection of gravitational waves from accreting neutron stars (NSs) in our Galaxy, due to
ellipticity or internal oscillation, would be a breakthrough in our understanding of compact …

Using Suzaku observations of three neutron star low-mass X-ray binaries (Ser X–1, 4U 1820–
30, and GX 349+ 2) we have found broad, asymmetric, relativistic Fe K emission lines in all …

The equation of state of cold baryonic matter is studied within a relativistic mean-field model
with hadron masses and coupling constants depending on the scalar field. All hadron …

In X-ray binaries, compact jets are known to commonly radiate at radio to infrared
frequencies, whereas at optical to γ-ray energies, the contribution of the jet is debated. The …

We have studied the atoll source 4U 1608-52 using a large data set obtained with the Rossi
X-Ray Timing Explorer. We find that the timing properties of 4U 1608-52 are almost exactly …

This lecture deals with aspects of the rapid X-ray variability of low-magnetic neutron stars in
low-mass X-ray binaries. After summarizing some basic considerations related to the …