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Highlights of Astronomy
Article
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Highlights of Astronomy
Article . 1998 . Peer-reviewed
License: Cambridge Core User Agreement
Data sources: Crossref
https://doi.org/10.1007/978-94...
Part of book or chapter of book . 1998 . Peer-reviewed
Data sources: Crossref
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Lte Models

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article 01 Jan 1998 English Publisher:Springer NetherlandsJournal:Highlights of Astronomy, volume 11, pages 646-649 (issn: 1539-2996, Copyright policy )
Authors: Robert L. Kurucz;

doi: 10.1007/978-94-011-4778-1_12 , 10.1017/s1539299600018347

Lte Models

Abstract

AbstractI can compute arbitrary-abundance models and spectra at high resolution using millions of atomic and diatomic molecular lines. Examples are given for Sakurai’s object and for a λBoo star. I am continuing to improve the input line data.

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    		 19
    popularity
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    influence
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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%
Average
bronze