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Multi-Color Observations of Young Star Clusters

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Conference object 01 Jan 2005Embargo end date: 01 Jan 2003 Germany English Publisher:Cambridge University Press (CUP)Journal:Highlights of Astronomy, volume 13, pages 195-195 (issn: 1539-2996, Copyright policy )
Authors: Anders, Peter; v. Alvensleben, Uta Fritze-; de Grijs, Richard;

doi: 10.1017/s1539299600015616 , 10.48550/arxiv.astro-ph/0309155

arXiv: http://arxiv.org/abs/astro-ph/0309155

Multi-Color Observations of Young Star Clusters

Abstract

AbstractWe present a new set of evolutionary synthesis models of our GALEV code, specifically developed to include the gaseous emission of presently forming star clusters, in combination with an advanced tool to compare large model grids with multi-color broad-band observations of YSC systems. Tests and first applications are presented.

Country
Germany
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Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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    influence
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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!
1
Average
Average
Average
Green
bronze
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