High-amplitude variable stars as MONS targets

Details High-amplitude variable stars as MONS targets High-amplitude variable stars as MONS targets

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000mons.proc..139c&link_type=abstract

The Third MONS Workshop: Science Preparation and Target Selection, Proceedings of a Workshop held in Aarhus, Denmark, January 24

Astronomy and Astrophysics

Astrophysics

Scientific paper

For a large number of variable stars MONS BST and FST will provide time series with a sensitivity in amplitude spectra orders of magnitude better than in data available until now. The very promising rewards of studying selected binary systems and classical high-amplitude variable stars with safe mode identification is emphasized. Several groups of binaries and of pulsation variables in the Cepheid instability strip as well as a few individual objects are discussed. Lists of variables of particular astrophysical importance as MONS targets are given.

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