New Findings about the S DOR Phenomenon

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Scientific paper

A century of photometric observations of AG Car and S Dor is investigated for general characteristics and possible periodicities in the occurrence of S Dor phases. We identify ``very-long-term" (VLT-SD) and ``normal" S Dor phases superimposed upon each other. The time scales for VLT-SD phases are about 25 and 35 years, and those for normal SD phases are 371 days and 6.8 years, respectively, for AG Car and S Dor. Further support has been found that the SD-phenomenon is due to a change in radius. No cyclic pattern (probably between 1 and 3 years according to photometry of the last 20 years) was found in the SD phases of eta Car, but there is evidence for a rising branch of a VLT-SD phase accompanying an ongoing decrease of the circumstellar dust density.

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