Properties of a Rapidly Rotating DME Star & of H-Alpha Anomalous Low-Mass Stars

Details Properties of a Rapidly Rotating DME Star & of H-Alpha Anomalous Low-Mass Stars Properties of a Rapidly Rotating DME Star & of H-Alpha Anomalous Low-Mass Stars

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iue..prop.1878s&link_type=abstract

IUE Proposal ID #CCGAS

Physics

Scientific paper

The issue of the effect of ultra-high rotation without attendant tidal effects on chromospheric and transition region signatures of dynamo activity in cool stars is to be examined by the observation of a recently discovered (Young, Skumanich and Harlan (1983), hereafter YSH83) rapidly rotating single dMe field star. In addition the chromospheric and transition region properties of stars found to be in a transition H-alpha emission state, i.e. between dMe and dM. YSH83 but with strong Ca+ chromospheres, will be determined. These observations will allow further study of the rotationactivity laws governing dynamo behaviour in solar-like stars as well as supplying needed constraints on chromospheric models for these stars.

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