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23 April 2024
 
  » arxiv » astro-ph/0011087

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Stellar Population analysis from Broad-Band Colours
Hamed Abdel-Hamid ; Peter Notni ;
Date 3 Nov 2000
Subject astro-ph
Affiliation National Research Institute of Astronomy and Geophysics, Egypt Astrophysikalisches Institut Potsdam, Germany
AbstractWe 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.
Source arXiv, astro-ph/0011087
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