683 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Brookhaven National LaboratoryUS12 papers
- Kent State UniversityUS12 papers
- Lawrence Berkeley National LaboratoryUS12 papers
- Purdue University West LafayetteUS12 papers
- Stony Brook UniversityUS12 papers
- The Ohio State UniversityUS12 papers
- University of California, DavisUS12 papers
- Carnegie Mellon UniversityUS11 papers
- Columbia UniversityUS11 papers
- Harbin Institute of TechnologyCN11 papers
- University of AucklandNZ11 papers
- University of Wisconsin–MadisonUS5 papers
6 papers · 1 filter
On the detection of Lorentzian profiles in a power spectrum: A Bayesian approach using ignorance priors
M. Gruberbauer, T. Kallinger, W. W. Weiss +1
Aims. Deriving accurate frequencies, amplitudes, and mode lifetimes from stochastically driven pulsation is challenging, more so, if one demands that realistic error estimates be g…
Conditions of Dynamical Stability for the HD 160691 Planetary System
Eric Bois, Ludmila Kiseleva-Eggleton, Nicolas Rambaux +1
The orbits in the HD 160691 planetary system at first appeared highly unstable, but using the MEGNO and FLI techniques of global dynamics analysis in the orbital parameter space we…
The Evolution of Cool Algols
Peter P. Eggleton, Ludmila Kiseleva-Eggleton
We apply a model of dynamo-driven mass loss, magnetic braking and tidal friction to the evolution of stars with cool convective envelopes; in particular we apply it to binary stars…
Global dynamics and stability limits for planetary systems around HD 12661, HD 38529, HD 37124 and HD 160691
Ludmila Kiseleva-Eggleton, Eric Bois, Nicolas Rambaux +1
In order to distinguish between regular and chaotic planetary orbits we apply a new technique called MEGNO in a wide neighbourhood of orbital parameters determined using standard t…
Evolution in Binary and Triple Stars, with an application to SS Lac
Peter P. Eggleton, Ludmila Kiseleva-Eggleton
We present equations governing the way in which both the orbit and the intrinsic spins of stars in a close binary should evolve subject to a number of perturbing forces, including…
Discovery of Extreme Examples of Superclustering in Aquarius
D. J. Batuski, C. J. Miller, K. A. Slinglend +5
We report the discovery of two highly extended filaments and one extremely high density knot within the region of Aquarius. The supercluster candidates were chosen via percolation…