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Cited article:
T. Schöning
Astron. Astrophys. Suppl. Ser., 122 2 (1997) 277-283
Published online: 1997-04-15
This article has been cited by the following article(s):
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Atomic data for neutron-capture elements
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THE ORIGIN AND EVOLUTION OF THE HALO PN BoBn 1: FROM A VIEWPOINT OF CHEMICAL ABUNDANCES BASED ON MULTIWAVELENGTH SPECTRA
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s‐Process Abundances in Planetary Nebulae
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The Abundances of Light Neutron‐Capture Elements in Planetary Nebulae. II.s‐Process Enrichments and Interpretation1
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s-process enrichment in the planetary nebula NGC 3918. Results from deep echelle spectrophotometry
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The Abundances of Light Neutron‐Capture Elements in Planetary Nebulae. I. Photoionization Modeling and Ionization Corrections
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THE ABUNDANCES OF LIGHT NEUTRON-CAPTURE ELEMENTS IN PLANETARY NEBULAE. III. THE IMPACT OF NEW ATOMIC DATA ON NEBULAR SELENIUM AND KRYPTON ABUNDANCE DETERMINATIONS
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Hunting for Planetary Nebulae toward the Galactic Center
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New atomic data for trans-iron elements and their application to abundance determinations in planetary nebulae1This review is part of a Special Issue on the 10th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas.
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Collisions of Electrons with Atomic Ions
A. K. Pradhan and H. L. Zhang
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DISCOVERY OF RUBIDIUM, CADMIUM, AND GERMANIUM EMISSION LINES IN THE NEAR-INFRARED SPECTRA OF PLANETARY NEBULAE
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Neutron-Capture Elements in Planetary Nebulae: Identification of Two Near-Infrared Emission Lines as [K[CLC]r[/CLC] [CSC]iii[/CSC]] and [S[CLC]e[/CLC] [CSC]iv[/CSC]]
Harriet L. Dinerstein
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