Observations and analysis of RW Dor.

Details Observations and analysis of RW Dor. Observations and analysis of RW Dor.

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soust..34...27m&link_type=abstract

South. Stars, Vol. 34, No. 3, p. 27 - 32

Physics

Scientific paper

Recent photometry of RW Dor at Auckland allow curve-fitting exercises to be carried out on the B and V data. Adequate curve fits can be produced by a pair of detached dwarfs, and while the primary may conform to a low mass mid-K type Main Sequence (MS) dwarf, in agreement with the known spectral and color classifications, the secondary would definitely be too hot for its mass as an MS object. The implication is thus that the model has some physical inadequacy.

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