POSTER PAPER 5.05
The FUSE Cool Star Survey
T. B. Ake, A. K. Dupree, J. L. Linsky, & the FUSE Cool Star Team
Institute: Department of Physics & Astronomy, Johns Hopkins University, Computer Sciences Corporation
Institute: Harvard-Smithsonian Center for Astrophysics
Institute: JILA, University of Colorado, and NIST
Contact Email: ake@pha.jhu.edu
Abstract:
As part of the PI-team program, the FUSE cool star group has surveyed
eight coronal, non-coronal, and hybrid stars using the LWRS (30"x30") aperture, providing full wavelength coverage in the FUSE bandpass. Additional stars are being observed with the MDRS
(4"x20") slit for the team D/H program,
primarily to obtain intrinsic Lyman Beta profiles. We provide here an
overview of the observations to date, with examples of the
types of studies currently in progress.
Index Keywords: Alpha Car
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Manuscript submitted: 2001-Sep-07
"The Future of Cool-Star Astrophysics", 2003, Eds. A. Brown,
G. M. Harper, & T. R. Ayres.
Proceedings of 12th Cambridge Workshop on Cool Stars, Stellar Systems,
& The Sun,
© 2003 University of Colorado.