H I FREE-BOUND EMISSION OF PLANETARY NEBULAE WITH LARGE ABUNDANCE DISCREPANCIES: TWO-COMPONENT MODELS VERSUS κ-DISTRIBUTED ELECTRONS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/780/i=1/a=93/pdf
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1. CAN SOLID BODY DESTRUCTION EXPLAIN ABUNDANCE DISCREPANCIES IN PLANETARY NEBULAE?
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4. Chemical abundances for Hf 2-2, a planetary nebula with the strongest-known heavy-element recombination lines
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