The MG II emission in BD -0 4234

Details The MG II emission in BD -0 4234 The MG II emission in BD -0 4234

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985obs...105...77r&link_type=abstract

The Observatory, vol. 105, p. 77-80 (1985)

Physics

2

Scientific paper

The strength of the Mg II emission in this metal-poor, high-velocity binary consisting of synchronized K-type dwarfs follows the same extension of the dependence on the inverse Rossby number which holds for rapidly-rotating Population I stars. This result indicates that the efficiency of the dynamo mechanism might be independent of metal abundance.

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