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Multiwavelength observations of ring galaxies. 2: Global star formation in ring galaxies
We present optical H-alpha emission-line images and K band near-infraredimages of a sample of collisionally formed ring galaxies. These are usedto determine the distribution of star formation and the distribution ofthe old stellar population, respectively, in the galaxies. Our resultsshow ring galaxies to have similar Hcx luminosities to starburstgalaxies, with star formation being contained almost exclusively in thering. In the larger ring galaxies we observe the ionized hydrogen to lieon the outer edge of the underlying, broader, K band ring. No conclusiveevidence is found in our sample for a true underlying stellar densitywave. Rather, the evidence suggests that either the density waves havepassed into the outer, mainly H I disk of the galaxies or that theprogenitor galaxies were mainly gas-rich low surface brightness objectsand that most of the optical/IR light we now observe has resulted fromrecent star formation in the expanding ring.
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Miembro de los siguientes grupos:
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Datos observacionales y astrométricos
| Constelación: | Tucán |
| Ascensión Recta: | 00h33m27.46s |
| Declinación: | -66°45'52.7" |
| Magnitud Aparente: | 9.924 |
| Movimiento Propio en Ascensión Recta: | 36.7 |
| Movimiento Propio en Declinación: | 2.4 |
| B-T magnitude: | 10.375 |
| V-T magnitude: | 9.962 |
Catálogos y designaciones:
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