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Paper detail

The Submillimetre Universe

Submillimetre continuum radiation allows us to probe cold objects, particularly the earliest, dusty phases of star formation, high-redshift galaxies and circumstellar disks. The submillimetre window gives a unique view of the physical and dynamical conditions in the neutral and molecular interstellar medium. In the next decade a combination of wide-field surveys with single-dish telescopes and targeted follow-up with ALMA and other facilities should enable rapid progress in answering questions about the origins of planetary systems, stars and galaxies.

preprint2010arXivOpen access
Douglas ScottPauline BarmbyPierre BastienJan CamiEdward ChapinJames Di FrancescoMichel FichMark HalpernMartin HoudeGilles JoncasDouglas JohnstonePeter MartinGaelen MarsdenBrenda MatthewsDavid NaylorC. Barth NetterfieldEls PeetersRene PlumeAlexandra PopeGerald SchievenTracy WebbChristine Wilson
astro-ph.IM
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Douglas ScottPauline BarmbyPierre BastienJan CamiEdward ChapinJames Di FrancescoMichel FichMark HalpernMartin HoudeGilles JoncasDouglas JohnstonePeter MartinGaelen MarsdenBrenda MatthewsDavid NaylorC. Barth NetterfieldEls PeetersRene PlumeAlexandra PopeGerald SchievenTracy WebbChristine Wilson

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