Workshop summary

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Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.238..137s&link_type=abstract

Astrophysics and Space Science, Volume 238, Issue 1, pp.137-140

Astronomy and Astrophysics

Astrophysics

Scientific paper

Observational phenomena correlated to planetary nebulae nuclei of the
Wolf-Rayet type have been analyzed in the framework of central star
evolution in general, and compared to the characteristics of classical
(Pop. I) WR stars.

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