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Table · dataset · 2007

Chemical abundances for Hf 2-2

Listed in IVOA Registry (Virtual Observatory)

We present high-quality optical spectroscopic observations of the planetary nebula (PN) Hf 2-2.

Description

The spectrum exhibits many prominent optical recombination lines (ORLs) from heavy-element ions. Analysis of the H I and He I recombination spectrum yields an electron temperature of ~900K, a factor of 10 lower than given by the collisionally excited [O III] forbidden lines.

The ionic abundances of heavy elements relative to hydrogen derived from ORLs are about a factor of 70 higher than those deduced from collisionally excited lines (CELs) from the same ions, the largest abundance discrepancy factor (adf) ever measured for a PN.

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Optical
Provenance · 1 source records, 9 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/mnras/368/195914 d agoJSON v1
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