Evolutionary status of hydrogen-deficient central stars of planetary
nebulae.
Gorny S.K., Tylenda R.
2000, A&A 362, 1008
Abstract:
-
The observational data for the planetary nebulae with hydrogen-deficient
central stars are analysed. We show that the general evolutionary sequence
is: late-[WC], early-[WC], PG 1159. An analysis of the observed
distributions of nebular parameters leads to a conclusion that the planetary
nebulae with hydrogen-deficient nuclei are not different from the population
of other planetary nebulae in the Galaxy. In particular the proportion of
the H-deficient stars among young nebulae is the same as in the whole
population. We have made a detailed comparison of the observed parameters
with theoretical modelling of the late He-shell flash (born again AGB)
scenario. Our finding is that the [WC] nuclei are not formed in a late
He-shell flash. This scenario can, however, give origin to some PG 1159
objects. There are five objects known which have presumably suffered from a
late He-shell flash. The observed parameters of their nebulae imply that
these stars will not become typical [WC] objects. Thus most of
hydrogen-deficient central stars (at least [WC]) evolve directly from the
AGB as do the other planetary nebula nuclei. We discuss implications of this
result.
PDF version of the paper is accessible via anonymous ftp:
gt00.pdf .
There is also a compressed PostScript
version. .
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