Understanding the γ Doradus Phenomenon using MONS

Details Understanding the γ Doradus Phenomenon using MONS Understanding the γ Doradus Phenomenon using MONS

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000mons.proc...91z&link_type=abstract

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

Physics

Scientific paper

We discuss the results expected from observing γ Dor stars with the MONS satellite. We first describe how the MONS Star Trackers will consistently improve the present knowledge of this new class of variables. We then discuss how the γ Dor can be considered possible "bridges" between opacity driven pulsations and stochastically excited solar like oscillations. For this reason the possible inclusion of a γ Dor representative in the MONS main target list is suggested and discussed. Three possible candidates are presented: γ Dor, 9 Aur and BS 2740.

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