activity
19952026
most citedAn absolutely calibrated effective temperature scale from the InfraRed Flux Method

724 citations · 11.7k across the 132 of their papers we have counts for

collaborators
Showing 2012Show all

15 papers · 1 filter

astro-ph.SR2012★ 68 cited

The Starburst Cluster Westerlund 1: The Initial Mass Function and Mass Segregation

Beomdu Lim, Moo-Young Chun, Hwankyung Sung +5

Westerlund 1 is the most important starburst cluster in the Galaxy due to its massive star content. We have performed BVIc and JKs photometry to investigate the initial mass functi…

astro-ph.SR2012★ 43 cited

The Initial Mass Function and the Surface Density Profile of NGC 6231

Hwankyung Sung, Hugues Sana, M. S. Bessell

We have performed new wide-field photometry of the young open cluster NGC 6231 to study the shape of the initial mass function (IMF) and mass segregation. We also investigated the…

astro-ph.GA2012★ 217 cited

The Most Metal-Poor Stars. IV. The Two Populations With [Fe/H] < -3.0

John E. Norris, David Yong, M. S. Bessell +8

We discuss the carbon-normal and carbon-rich populations of Galactic halo stars having [Fe/H] < -3.0, utilizing chemical abundances from high-resolution, high-S/N model-atmosphere…

astro-ph.SR2012★ 75 cited

A High-Resolution Spectroscopic Search for the Remaining Donor for Tycho's Supernova

Wolfgang E. Kerzendorf, David Yong, Brian P. Schmidt +12

In this paper, we report on our analysis using Hubble Space Telescope astrometry and Keck-I HIRES spectroscopy of the central six stars of Tycho's supernova remnant (SN 1572). With…

astro-ph.SR2012★ 45 cited

Identifying Nearby, Young, Late-type Stars by Means of Their Circumstellar Disks

Adam Schneider, Inseok Song, Carl Melis +2

It has recently been shown that a significant fraction of late-type members of nearby, very young associations (age <10 Myr) display excess emission at mid-IR wavelengths indicativ…

astro-ph.SR2012★ 14 cited

Deep search for companions to probable young brown dwarfs

G. Chauvin, J. Faherty, A. Boccaletti +10

We have obtained high contrast images of four nearby, faint, and very low mass objects 2MASSJ04351455-1414468, SDSSJ044337.61+000205.1, 2MASSJ06085283-2753583 and 2MASSJ06524851-57…