Results 21 to 30 of about 2,099,705 (77)
Probing the composition of sub-millisecond rotating compact stars by r-modes instability [PDF]
We investigate the implications of the r-modes instability on the composition of a compact star rotating at a sub-millisecond period. In particular, the only viable astrophysical scenario for such an object, wich might present inside the Low Mass X-ray ...
Giuseppe Pagliara +3 more
core +1 more source
Accretion processes in AM Herculis systems [PDF]
We begin by presenting a theoretical model for the radial velocity and velocity dispersion of the broad emission line component in AM Herculis systems assuming that it originates mainly in the gas which is diverted out of the orbital plane and ...
Ferrario, L.
core +1 more source
Gravitoastronomy with neutron stars [PDF]
Recent advances in gravitational wave detectors mean that we can start to make astrophysically important statements about the physics of neutron stars based on observed upper limits to their gravitational luminosity.
Woan, G., Graham Woan
core +1 more source
Infrared and optical polarimetry of AM Herculis
Circular polarization observations of AM Herculis have been obtained at wavelengths from 0.55 micron (V) to 2.2 micron (K) using a simultaneous three-channel polarimeter.
Axon, D.J. +3 more
core +4 more sources
A recent development in the study of magnetic cataclysmic variable stars (mCVs) has been the identification of asynchronously spinning mCVs with orbital periods
Colin Littlefield +4 more
doaj +1 more source
Studies on the Habits and Distribution of Cryptocerus Texanus Santschi (Hymenoptera: Formicidae)
Psyche: A Journal of Entomology, Volume 61, Issue 2, Page 41-57, 1954.
W. S. Creighton, R. E. Geegg
wiley +1 more source
Energy Transport in Radially Accreting White Dwarf Stars [PDF]
AM Herculis stars form a subclass of cataclysmic variables, the defining characteristic of which is that they possess a high degree of polarisation at optical frequencies. Physically they have two notable features.
Thompson, Alan McLure
core +5 more sources
Wide binary stars in the Galactic field : a statistical approach [PDF]
This thesis focuses on the statistical properties of wide binary (WB) star systems in the Galactic field. With projected separations larger than 200 AU and, consequently, having very low binding energies, WB are sensitive probes of the Galactic ...
Longhitano, Marco
core +1 more source
EXO 023432-5232.3 - an eclipsing AM Herculis binary
The authors report observations of the serendipitous EXOSAT source EXO 023432-5232.3 which confirm that the object is an AM Herculis type binary and show the presence of eclipses by the companion star.
Wickramasinghe, D.T. +3 more
core +4 more sources
Pulsation versus metallicism in Am stars as revealed by LAMOST and WASP [PDF]
We present the results of a study of a large sample of A and Am stars with spectral types from LAMOST and light curves from WASP. We find that, unlike normal A stars, δ Sct pulsations in Am stars are mostly confined to the effective temperature range ...
R. Anderson, D. +48 more
core +3 more sources

