SIMBAD references

1999MNRAS.306..806S - Mon. Not. R. Astron. Soc., 306, 806-808 (1999/July-2)

Detecting planets in planetary nebulae.

SOKER N.

Abstract (from CDS):

We examine the possibility of detecting signatures of surviving Uranus/Neptune-like planets inside planetary nebulae. Planets that are not too close to the stars (orbital separation larger than ∼5au) are likely to survive the entire evolution of the star. As the star turns into a planetary nebula, it has a fast wind and strong ionizing radiation. The interaction of the radiation and wind with a planet may lead to the formation of a compact condensation or tail inside the planetary nebula, which emits strongly in Hα, but not in [Oiii]. The position of the condensation (or tail) will change over a time-scale of ∼10yr. Such condensations might be detected with currently existing telescopes.

Abstract Copyright: 1999 RAS

Journal keyword(s): stars: AGB and post-AGB - binaries: close - planetary systems - planetary nebulae: general

Simbad objects: 5

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