The metal contents of two groups of galaxies
Context. The hot gas in clusters and groups of galaxies is continuously being enriched with metals from supernovae and stars. It is well established that the enrichment of the gas with elements from oxygen to iron is mainly caused by supernova explosions. The origins of nitrogen and carbon are still...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2011-07, Vol.531, p.A15 |
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Hauptverfasser: | , , , , , , |
Format: | Artikel |
Sprache: | eng |
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