Starburst Galaxies

dc.creatorMuxlow, T. W. B.
dc.creatorBeswick, R. J.
dc.creatorRichards, A. M. S.
dc.creatorThrall, H.
dc.date2006-11-30
dc.date.accessioned2026-07-07T07:31:02Z
dc.date.available2026-07-07T07:31:02Z
dc.descriptionStar-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.
dc.description15 pages, 19 figures, To appear in the proceedings of `The 8th European VLBI Network Symposium on New Developments in VLBI Science and Technology', ed. A. Marecki et al., held in Torun, Poland, on September 26-29, 2006 (Invited Review)
dc.identifierhttps://arxiv.org/abs/astro-ph/0611951
dc.identifierhttp://arxiv.org/abs/astro-ph/0611951
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118609
dc.subjectAstrophysics
dc.titleStarburst Galaxies
dc.typetext

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