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Introduction to the JCMT-CSO Interferometer

Wiedner, M. C. and Hills, R. E. and Carlstrom, J. E. and Lay, O. P. (1996) Introduction to the JCMT-CSO Interferometer. In: New Light on Galaxy Evolution. IAU Symposium Proceedings Series. No.171. Kluwer , Dordrecht, p. 467. ISBN 9780792339755. http://resolver.caltech.edu/CaltechAUTHORS:20181211-073511185

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Abstract

The James Clerk Maxwell Telescope (JCMT) and the Caltech Submillimeter Observatory (CSO) are located 160m apart on Mauna Kea, Hawaii. Recently they have been linked together to allow the first submillimetre interferometric observations (between 300GHz and 490GHz, soon to 690GHz). Submillimetre observations can be used to probe the physical conditions of molecular clouds and dust in starforming regions. Lines from rotational transitions of molecules such as CO, HCN and HCO+ trace densities, temperatures and masses of molecular gas. The thermal emission of cold dust, typically found in dense clouds, also peaks in the submm regime.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1017/S0074180900233858DOIArticle
Additional Information:© 1996 Kluwer.
Record Number:CaltechAUTHORS:20181211-073511185
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20181211-073511185
Official Citation:Wiedner, M., Hills, R., Carlstrom, J., & Lay, O. (1996). Introduction to the JCMT-CSO Interferometer. Symposium - International Astronomical Union, 171, 467-467. doi:10.1017/S0074180900233858
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:91664
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:11 Dec 2018 19:43
Last Modified:11 Dec 2018 22:10

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