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Astrophysics and Space Science
Article . 1969 . Peer-reviewed
License: Springer TDM
Data sources: Crossref
https://dx.doi.org/10.1007/bf0...
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Tentative identification of the diffuse interstellar absorption bands and of a diffuse interstellar doublet line

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1969 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 3, pages 102-108 (issn: 0004-640X, eissn: 1572-946X, Copyright policy )
Authors: Mogens Rudkj�bing;

doi: 10.1007/bf00649596

Tentative identification of the diffuse interstellar absorption bands and of a diffuse interstellar doublet line

Abstract

The four diffuse interstellar absorption bands at λ4430, λ4760, λ4890, and λ6180 and the two diffuse lines at λ5780 and λ5797 are interpreted as belonging to pre-ionization transitions in H− and O−, respectively. In both cases the identifications are supported by extrapolations of wave numbers of resonance lines along isoelectronic sequences.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
19
Average
Top 10%
Top 10%
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