Thirty Years of Star Formation at UKIRT

Conference paper
First Online:
Part of the Astrophysics and Space Science Proceedings book series (ASSSP, volume 37)

Abstract

It’s safe to say that UKIRT’s contribution to star formation at near-infrared (near-IR), mid-infrared (mid-IR) and even sub-millimetre (sub-mm) wavelengths has been considerable. From the early days of single-detector photometers, through the development of 2-D arrays and complex multi-mode imager-spectrometers, to the present-day large-format imager WFCAM, UKIRT has offered the international community access to some of the world’s most innovative, competitive, and versatile instrumentation possible. Suffice to say, UKIRT users have made the most of these instruments! Below I try to give a taste of the variety of star formation research that has come to pass at UKIRT (with apologies to those whose important work I fail to mention).

Keywords

Star Formation Young Star Tauri Star Queen Mary College Molecular Outflow 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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Copyright information

© Springer Science+Business Media Dordrecht 2013

Authors and Affiliations

  1. 1.Astrophysics Research Institute, Liverpool John Moores UniversityBrownlow Hill LiverpoolUK

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