collaborators

6 papers

astro-ph.SR20091 cited

Tidal effects and periastron events in binary stars

Gloria Koenigsberger, Edmundo Moreno

Binary stars in eccentric orbits are frequently reported to present increasing levels of activity around periastron passage. In this paper we present results of a calculation from…

astro-ph.SR2009

Tidal Flows from Asynchronous Rotation in Binaries

Gloria Koenigsberger, Edmundo Moreno, David Harrington

Asynchronous rotation in binary stars produces non-radial oscillations that are known to cause observable variability on orbital timescales. The horizontal perturbations of the sur…

astro-ph200726 cited

First detection of phase-dependent colliding wind X-ray emission outside the Milky Way

Yael Naze, Michael F. Corcoran, Gloria Koenisgberger +1

After having reported the detection of X-rays emitted by the peculiar system HD5980, we assess here the origin of this high-energy emission from additional X-ray observations obtai…

astro-ph200639 cited

Tides in asynchronous binary systems

Oswaldo Toledano, Edmundo Moreno, Gloria Koenigsberger +2

Stellar oscillations are excited in non-synchronously rotating stars in binary systems due to the tidal forces. Tangential components of the tides can drive a shear flow which beha…

astro-ph200638 cited

The X-ray binary 2S0114+650=LSI+65 010:A slow pulsar or tidally-induced pulsations?

G. Koenigsberger, L. Georgiev, E. Moreno +3

The X-ray source 2S0114+650=LSI+65 010 is a binary system containing a B-type primary and a low mass companion believed to be a neutron star. The system has three reported periodic…

astro-ph200613 cited

FUSE observations of HD 5980: The wind structure of the eruptor

Gloria Koenigsberger, Alexander W. Fullerton, Derck Massa +1

HD 5980 is a unique system containing one massive star (star A) that is apparently entering the luminous blue variable phase, and an eclipsing companion (star B) that may have alre…