2.3. Old Population 2.4. Magnetic Fields of Neutron Stars 2.5. Z and Atoll Classification 3.
Type I X-ray Bursts 3.1. Introduction 3.2. Burst Profiles 3.3. Burst Spectral Analysis 3.4 …

There is a class of bright (~> 1034 ergs s-1) X-ray sources which distinguish themselves
from the massive X-ray binaries by the following characteristics:-Their star-like optical …

We examined the maximum bolometric peak luminosities during type I X-ray bursts from the
persistent or transient luminous X-ray sources in globular clusters. We show that for about …

Neutron Stars in Interacting Binary Systems ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …

Thermonuclear processes on accreting neutron stars - A systematic study ADS Classic is now
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …

Precise and reliable measurements of the masses and radii of neutron stars with a variety of
masses would provide valuable guidance for improving models of the properties of cold …

Simultaneous, precise measurements of the mass M and radius R of neutron stars can yield
uniquely valuable information about the still uncertain properties of cold matter at several …

Measurement of at least three independent parameters, for example, mass, radius and spin
frequency, of a neutron star is probably the only way to understand the nature of its …

The angular distribution and polarization of radiation from X-ray bursters have been
calculated. It is shown that the accretion disc around the neutron star intercepts and re …

Aims. We explore the accretion disk and boundary layer emission in bright neutron star
LMXBs and their dependence on the mass accretion rate. Methods. We used Fourier …