389 citations
- Carnegie ObservatoriesUS10 papers
- Geophysical LaboratoryUS7 papers
- California Institute of TechnologyUS4 papers
- Leiden UniversityNL3 papers
- The University of Texas at AustinUS3 papers
- Bhabha Atomic Research CentreIN2 papers
- Center for Astrophysics Harvard & SmithsonianUS2 papers
- Jet Propulsion LaboratoryUS2 papers
- National Astronomical Observatory of JapanJP2 papers
- Osservatorio Astronomico di PadovaIT2 papers
- Princeton Public SchoolsUS2 papers
- Princeton UniversityUS2 papers
9 papers · 1 filter
Oscillations in Procyon A: First results from a multi-site campaign
S. Hekker, T. Arentoft, H. Kjeldsen +45
Procyon A is a bright F5IV star in a binary system. Although the distance, mass and angular diameter of this star are all known with high precision, the exact evolutionary state is…
The SEGUE Stellar Parameter Pipeline. III. Comparison with High-Resolution Spectroscopy of SDSS/SEGUE Field Stars
C. Allende Prieto, T. Sivarani, T. C. Beers +14
We report high-resolution spectroscopy of 125 field stars previously observed as part of the Sloan Digital Sky Survey and its program for Galactic studies, the Sloan Extension for…
Prediction of polar ordered oxynitride perovskites
Razvan Caracas, R. E. Cohen
Using a materials by design approach, the authors find a class of ordered oxynitride piezoelectrics with perovskite structure. They predict that ordered YSiO2N and YGeO2N are chara…
The Spitzer 24-micron Photometric Light Curve of the Eclipsing M-dwarf Binary GU Bootis
Kaspar von Braun, Gerard T. van Belle, David Ciardi +3
We present a carefully controlled set of Spitzer 24 \micron MIPS time series observations of the low mass eclipsing binary star GU Boötis (GU Boo). Our data cover three secondary e…
N-body integrators for planets in binary star systems
John E. Chambers
Symplectic integrators are the tool of choice for many researchers studying dynamical systems because of their good long-term energy conservation properties. For systems with a dom…
Gravitational instability in binary protoplanetary disks
Lucio Mayer, Alan Boss, Andrew F. Nelson
We review the models and results of simulations of self-gravitating, gaseous protoplanetary disks in binary star systems. These models have been calculated by three different group…