Spectral analysis of the barium central star of the planetary nebula Hen 2-39
Context. Barium stars are peculiar red giants characterized by an overabundance of the elements synthesized in the slow neutron-capture nucleosynthesis (s-process elements) along with an enrichment in carbon. These stars are discovered in binaries with white dwarf companions. The more recently formed of these stars are still surrounded by a
Löbling, L. et al.
Fecha de publicación:
4
2019