PI: Carl Melis, UC San Diego, email@example.com
Address: Center for Astrophysics and Space Sciences, 9500 Gilman Drive, Code 0424, La Jolla, CA, 92093-0424 USA
CoI: Guillermo Torres, Harvard-Smithsonian Center for Astrophysics
Title: A Search for Pre-Main Sequence Spectroscopic Binaries in the Pleiades
Abstract: We propose Gemini/GRACES spectroscopic observations of M-type Pleiades stars whose low mass and young age place them in the pre-main sequence evolutionary phase. The collection of measurements produced by this proposal will provide new stress tests for stellar physical models and pave the way for a future Pleiades mass measuring program that focuses on a major discrepancy between models and observations of young, low mass stars. The search for low-mass stellar multiple systems in the Pleiades cluster will also bridge efforts that largely have focused on identifying binary companions of stellar members of Solar-mass and above or substellar objects in the cluster.
Program Type: Standard/Galactic
Run 1 (2017B): GEM-N-SVC/GRACES -- 31.2hrs band 2 (GN-2017B-Q-48)
National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360