Abstract
We summarize results of arcsecond and milliarcsecond-resolution radio imaging of starbursts. Thermal radio emission from young super star clusters (SSCs) indicates that they are powered by the equivalent of hundreds to thousands of 07 stars. Milliarcsecond imaging of Arp 299 reveals individual young supernovae that are factors of similar to 100 more powerful than Cas A, and that may show the locations of older SSCs in which the most massive stars already have gone supernova.
Cite
CITATION STYLE
Ulvestad, J. S. (2005). Compact Extragalactic Star Formation: Peering through the Dust at Centimeter Wavelengths. In Starbursts (pp. 127–132). Springer Netherlands. https://doi.org/10.1007/1-4020-3539-x_22
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