output
20032026
most citedBrownian distance covariance

857 citations

Showing 2007 · astro-phShow all

8 papers · 2 filters

astro-ph2007★ 70 cited

Rotation and Macroturbulence in Metal-poor Field Red Giant and Red Horizontal Branch Stars

Bruce W. Carney, David F. Gray, David Yong +4

We report the results for rotational velocities, Vrot sin i, and macroturbulence dispersion, zeta(RT), for 12 metal-poor field red giant branch stars and 7 metal-poor field red hor…

astro-ph2007

Observational Tests of Planet Formation Models

A. Sozzetti, G. Torres, D. W. Latham +8

We summarize the results of two experiments to address important issues related to the correlation between planet frequencies and properties and the metallicity of the hosts. Our r…

astro-ph2007★ 14 cited

Modeling the Galactic CV Distribution for the ChaMPlane Survey

A. B. Rogel, H. N. Cohn, P. M. Lugger

For purposes of designing targeted cataclysmic variable (CV) detection surveys and interpreting results of other projects with many CV detections such as the ChaMPlane Survey, we h…

astro-ph2007★ 30 cited

Line Broadening in Field Metal-poor Red Giant and Red Horizontal Branch Stars

Bruce W. Carney, David W. Latham, R. P. Stefanik +1

We report 349 radial velocities for 45 metal-poor field red giant and red horizontal branch stars. We have have identified one new spectroscopic binary, HD 4306, and one possible s…

astro-ph2007★ 26 cited

Discovery of Gas Accretion Onto Stars in 13 Myr old h and chi Persei

Thayne Currie, Scott Kenyon, Zoltan Balog +2

We report the discovery of accretion disks associated with ~ 13 Myr-old intermediate/low-mass stars in h and chi Persei. Optical spectroscopy of ~ 5000 stars in these clusters and…

astro-ph2007★ 102 cited

The Rise and Fall of Debris Disks: MIPS Observations of h and chi Persei and the Evolution of Mid-IR Emission from Planet Formation

Thayne Currie, Scott Kenyon, Zoltan Balog +3

We describe Spitzer/MIPS observations of the double cluster, h and Persei, covering a 0.6 square-degree area surrounding the cores of both clusters. The data are combine…