Observing B-type pulsators with MONS

Details Observing B-type pulsators with MONS Observing B-type pulsators with MONS

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000mons.proc...59a&link_type=abstract

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

Computer Science

Scientific paper

We overview the different classes of B-type pulsators and show from our ground-based data that current data sets are insufficient to derive the complete frequency spectrum. From line-profile studies, we find that many modes with small amplitudes are excited in some stars, of which extensive ground-based photometry has revealed only one frequency. MONS data of such objects would offer a unique opportunity to perform seismology in massive stars that are situated along the main sequence.

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