activity
20052009
most citedThe Chemical Evolution of the Draco Dwarf Spheroidal Galaxy

213 citations · 383 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.SR200943 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.GA2009213 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.SR200929 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-ph200857 cited

Clues to the Metallicity Distribution in the Galactic Bulge: Abundances in OGLE-2007_BLG-349S

Judith G. Cohen, Wenjin Huang, A. Udalski +2

We present an abundance analysis based on high dispersion and high signal-to-noise ratio Keck spectra of a very highly microlensed Galactic bulge dwarf, OGLE-2007-BLG-349S, with Te…

astro-ph200741 cited

The B and Be Star Population of NGC 3766

M. Virginia McSwain, Wenjin Huang, Douglas R. Gies +2

We present multiple epochs of H-alpha spectroscopy for 47 members of the open cluster NGC 3766 to investigate the long term variability of its Be stars. Sixteen of the stars in thi…

astro-ph2005

Stellar Rotation in Young Clusters. II. Evolution of Stellar Rotation and Surface Helium Abundance

W. Huang, D. R. Gies

We derive the effective temperatures and gravities of 461 OB stars in 19 young clusters by fitting the H-gamma profile in their spectra. We use synthetic model profiles for rotatin…