Targets for MONS: gamma DOR stars, Be stars and T Tauri stars, and the capabilities of ground-based support observing

Details Targets for MONS: gamma DOR stars, Be stars and T Tauri stars, and the capabilities of ground-based support observing Targets for MONS: gamma DOR stars, Be stars and T Tauri stars, and the capabilities of ground-based support observing

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mons.proc..141l&link_type=abstract

The First MONS Workshop: Science with a Small Space Telescope, held in Aarhus, Denmark, June 29 - 30, 1998, Eds.: H. Kjeldsen, T

Astronomy and Astrophysics

Astrophysics

Scientific paper

Designed to detect micro-magnitude amplitude solar-like oscillations in bright solar-type stars, MONS can significantly out-perform ground-based photometric telescopes and thus has the capability to generate exciting new astrophysics for a wide variety of stellar types. Several types of stars not represented on the preliminary target list that would benefit from MONS observations are considered.

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