activity
20052012
most citedA Stellar Rotation Census of B Stars: from ZAMS to TAMS

265 citations · 1.4k across the 20 of their papers we have counts for

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Showing 2009Show all

6 papers · 1 filter

astro-ph.GA2009★ 13 cited

A Puzzle Involving Galactic Bulge Microlensing Events

Judith G. Cohen, Andrew Gould, Ian B. Thompson +7

We study a sample of 16 microlensed Galactic bulge main sequence turnoff region stars for which high dispersion spectra have been obtained with detailed abundance analyses. We demo…

astro-ph.SR2009

HD 69686: A Mysterious High Velocity B Star

Wenjin Huang, Douglas R. Gies, M. Virginia McSwain

We report on the discovery of a high velocity B star, HD 69686. We estimate its space velocity, distance, surface temperature, gravity, and age. With these data, we are able to rec…

astro-ph.SR2009★ 43 cited

Variability of Be Stars in Southern Open Clusters

M. Virginia McSwain, Wenjin Huang, Douglas R. Gies

We recently discovered a large number of highly active Be stars in the open cluster NGC 3766, making it an excellent location to study the formation mechanism of Be star disks. To…

astro-ph.GA2009★ 213 cited

The Chemical Evolution of the Draco Dwarf Spheroidal Galaxy

Judith G. Cohen, Wenjin Huang

We present an abundance analysis based on high resolution spectra of 8 stars selected to span the full range in metallicity in the Draco dwarf spheroidal galaxy. We find [Fe/H] for…

astro-ph.SR2009★ 29 cited

Clues to the Metallicity Distribution in the Galactic Bulge: Abundances in MOA-2008-BLG310 and MOA-2008-BLG311

Judith G. Cohen, Ian B. Thompson, Takahiro Sumi +5

We present abundance analyses based on high dispersion and high signal-to-noise ratio Magellan spectra of two highly microlensed Galactic bulge stars in the region of the main sequ…

astro-ph.GA2009★ 30 cited

Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. Detailed abundance analysis of OGLE-2008-BLG-209S

T. Bensby, J. A. Johnson, J. Cohen +7

AIMS. Our aims are twofold. First we aim to evaluate the robustness and accuracy of stellar parameters and detailed elemental abundances that can be derived from high-resolution sp…