Abstract
We describe studies of star formation in various galaxies using primarily observations from the Wise Observatory. In addition to surface photometry in the broad band UBVRI, we also use a set of narrow-band H-alpha filters tuned to different redshifts to isolate the emission line. With these observational data, and using models of evolutionary stellar populations, we unravel the star formation histories of the galaxies and connect them to other parameters, such as the galaxy environment.
| Original language | English |
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| State | Published - 2008 |
| Event | Poster paper at the First Middle East-Africa IAU Regional Meeting, Cairo (Egypt), May 2008 - Cairo, Egypt Duration: 5 Apr 2008 → 10 Apr 2008 |
Conference
| Conference | Poster paper at the First Middle East-Africa IAU Regional Meeting, Cairo (Egypt), May 2008 |
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| Country/Territory | Egypt |
| City | Cairo |
| Period | 5/04/08 → 10/04/08 |
Keywords
- astro-ph