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

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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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