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Symposium - International Astronomical Union
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Symposium - International Astronomical Union
Article . 1996 . Peer-reviewed
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Article . 2009 . Peer-reviewed
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Star and Globular Cluster Formation in Mergers

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type 01 Jan 1996 United Kingdom Publisher:Cambridge University Press (CUP)Journal:Symposium - International Astronomical Union, volume 171, pages 376-376 (issn: 0074-1809, Copyright policy )
Authors: Fritze, U.;

doi: 10.1017/s0074180900232956

handle: 2299/3305

Star and Globular Cluster Formation in Mergers

Abstract

The high burst strengths and star formation efficiencies found with spectrophotmetric and chemical evolutionary synthesis for mergers of gas-rich spirals led us to expect the formation of a secondary population of globular clusters (GC) with enhanced metallicity (F. – v. A. & Gerhard 1994, A&A 285, 751 u.775). HST imaging of NGC 7252, NGC 4038/39 and NGC 1275 revealed rich populations of bright young star clusters (YSC).

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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!
0
Average
Average
Average
bronze
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