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arXiv · astro-ph/0011087

Stellar Population analysis from Broad-Band Colours

Hamed Abdel-Hamid·Peter Notni
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Abstract

We have developed an analytical method to investigate the stellar populations in a galaxy using the broad-band colours. The method enables us to determine the relative contribution, spatial distribution and age for different stellar populations and gives a hint about the dust distribution in a galaxy. We apply this method to the irregular galaxy NGC 3077, using CCD images in U, B, V and R filters.

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Hamed Abdel-Hamid, Peter Notni. 2000-11-23. Stellar Population analysis from Broad-Band Colours. https://doi.org/10.1002/1521-3994(200012)321%3A5%2F6%3C307%3A%3Aaid-asna307%3E3.0.co%3B2-4

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