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Starburst Galaxies

T. W. B. Muxlow·R. J. Beswick·A. M. S. Richards·H. Thrall
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Abstract

Star-formation and the Starburst phenomenon are presented with respect to a number of nearby star-forming galaxies where our understanding of the process can be calibrated. Methods of estimating star-formation rates are discussed together with the role played in the investigation of the process by multi-wavelength studies of a few selected starburst galaxies (especially the well studied galaxy M82). Our understanding of nearby systems allows us to study the star-formation history of the Universe by observing high-redshift starburst galaxies. These begin to dominate the radio source populations at centimetric wavelengths at flux densities below a few 10s of Jy. New very sensitive, high resolution telescopes in the sub-mm and radio will revolutionize our understanding of these distant star-forming systems, some of which may contain embedded AGN.

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T. W. B. Muxlow, R. J. Beswick, A. M. S. Richards, H. Thrall. 2006-11-30. Starburst Galaxies. https://arxiv.org/abs/astro-ph/0611951

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