(Q58917019)

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Testing stellar population models with star clusters in the Large Magellanic Cloud

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Testing stellar population models with star clusters in the Large Magellanic Cloud (English)

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2

Fiona Hoyle

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Michael A. Beasley

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1

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Ray M. Sharples

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3

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English

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publication date

October 2002

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number of pages

21 page

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Monthly Notices of the Royal Astronomical Society

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volume

336

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1

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168–188

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cites work

Ages and metallicities of globular clusters in NGC 4472

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Crossref

reference URL

https://api.crossref.org/works/10.1046%2FJ.1365-8711.2002.05714.X

retrieved

21 January 2018

Distances, Ages, and Epoch of Formation of Globular Clusters

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Crossref

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https://api.crossref.org/works/10.1046%2FJ.1365-8711.2002.05714.X

retrieved

21 January 2018

The Ages and Abundances of a Large Sample of M87 Globular Clusters

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Crossref

reference URL

https://api.crossref.org/works/10.1046%2FJ.1365-8711.2002.05714.X

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21 January 2018

Age Estimates for Globular Clusters in NGC 1399

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Crossref

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https://api.crossref.org/works/10.1046%2FJ.1365-8711.2002.05714.X

retrieved

21 January 2018

Keck Spectroscopy of Globular Clusters around NGC 1399

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https://api.crossref.org/works/10.1046%2FJ.1365-8711.2002.05714.X

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21 January 2018

On the dependence of spectroscopic indices of early-type galaxies on age, metallicity and velocity dispersion

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reference URL

https://api.crossref.org/works/10.1046%2FJ.1365-8711.2002.05714.X

retrieved

21 January 2018

Strong Balmer Lines in Old Stellar Populations: No Need for Young Ages in Ellipticals?

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Crossref

reference URL

https://api.crossref.org/works/10.1046%2FJ.1365-8711.2002.05714.X

21 January 2018

1 reference

https://api.crossref.org/works/10.1046%2FJ.1365-8711.2002.05714.X

retrieved

21 January 2018

The AGB phase-transition outside the local group:K-band observations of young star clusters in NGC 7252

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stated in

Crossref

reference URL

https://api.crossref.org/works/10.1046%2FJ.1365-8711.2002.05714.X

retrieved

21 January 2018

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10.1046/J.1365-8711.2002.05714.X

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(Q58917019)

Testing stellar population models with star clusters in the Large Magellanic Cloud

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