Abstract
We examine light curves obtained for several low-mass subluminous [WC] central stars. Recent visual and photoelectric measurements made of the [WC10] central star CPD-56°8032 indicate that it has undergone a second decline event resembling those seen in the R Coronae Borealis (RCB) variables. Other [WC] central stars examined (He2-113, SwSt1, and He2-99) do not show declines. Various evolutionary scenarios have been proposed that link the [WC] stars, RCB stars, and other types of hydrogen-deficient objects. From an observational point of view, the evidence appears to be circumstantial.
Original language | English |
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Pages (from-to) | 76-80 |
Number of pages | 5 |
Journal | Observatory |
Volume | 119 |
Issue number | 1149 |
Publication status | Published - Apr 1999 |