The FUSE Cool Star Survey

Details The FUSE Cool Star Survey The FUSE Cool Star Survey

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003csss...12..857a&link_type=abstract

The Future of Cool-Star Astrophysics: 12th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (2001 July 30 - August

Astronomy and Astrophysics

Astrophysics

Α Car

Scientific paper

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 arcsec × 30 arcsec) aperture, providing full wavelength coverage in the FUSE bandpass. Additional stars are being observed with the MDRS (4 arcsec × 20 arcsec) slit for the team D/H program, primarily to obtain intrinsic Lyman β profiles. We provide here an overview of the observations to date, with examples of the types of studies currently in progress.

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