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International Astronomical Union Colloquium
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International Astronomical Union Colloquium
Article . 1997 . Peer-reviewed
License: Cambridge Core User Agreement
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https://doi.org/10.1007/bfb010...
Part of book or chapter of book . 2008 . Peer-reviewed
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Evolution of evolution of superbubbles

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Other literature type 01 Jan 1997 English Publisher:Springer Berlin HeidelbergJournal:International Astronomical Union Colloquium, volume 166, pages 397-407 (issn: 0252-9211, Copyright policy )
Authors: Satoru Ikeuchi;

doi: 10.1007/bfb0104754 , 10.1017/s0252921100071323

Evolution of evolution of superbubbles

Abstract

AbstractIn the first place, I will summarize the evolution of our picture of the ISM over the past several decades in order to see the importance of superbubbles for ISM structure. In accordance with the progress of observations, the picture of the ISM has dramatically changed from the 1960s. Then, I will review the evolution of theoretical models of superbubbles including the idea of chimney structures of the ISM.

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citations
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!
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Average
Average
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