Lee Hartmann

TL;DR: In this article, the inner scattered light structure of L1527 IRS (IRAS 04368+2557) was resolved in the Gemini image into a compact bipolar structure with a narrow dark lane in the center, which is consistent with the initial modeling of a bright inner cavity separated by a dark lane due to extinction along the line of sight of the central protostar by the disk.

TL;DR: This paper examined the spectroscopic binary population for two massive nearby regions of clustered star formation, the Orion Nebula Cluster (ONC) and NGC 2264, supplementing the data presented by Tobin et al. with more recent observations and more extensive analysis.

TL;DR: In this article, the authors used the Extreme Science and Engineering Discovery Environment (XSEDE), which was supported by National Science Foundation grant number ACI-1053575, to provide HPC resources that have contributed to the research results reported within this paper.

TL;DR: The Coordinated Synoptic Investigation of NGC 2264 (CSI 2264) as mentioned in this paper was a 30-day multi-wavelength photometric monitoring campaign on more than 1000 young star members using 16 telescopes.

TL;DR: In this article, the authors present optical, IR and millimeter observations of the solar-type star 13-277, also known as GM Cep, in the 4 Myr-old cluster Tr 37.