White, Glenn J.; Rainey, Ruth; Avery, Lorne; Phillips, Peter; Griffin, Matthew; Monteiro, Tania; Richardson, Kevin; Cronin, Nigel and Harten, Ron
Due to copyright restrictions, this file is not available for public download
|Google Scholar:||Look up in Google Scholar|
We report on extensive submillimetre wavelength observations in the CO J=3-2 and 4-3 lines towards a sample of star formation regions. The observations have been obtained using the Queen Mary college Submillimetre Heterodyne Receiver at the UKIRT 3.8 m telescope. The data include observations and maps of NGC 2024, S88, W3, S140, CRL2591, NGC 2264, K3-50, G35.2-0.74, ρ Oph A, M17, W51, S68, S106, NGC 1333, DR21 and W49. Several new bipolar flow sources have been detected in NGC 2024, S88 and NGC 2264. Comparisons between the spectra in the CO J=1-0, 2-1, 3-2 and 4-3 transitions will be discussed in terms of their excitation, in particular for the gas in the high velocity line wings, where we have attempted to estimate the densities and relative abundances of the flow material.
|Item Type:||Conference Item|
|Copyright Holders:||1987 International Astronomical Union|
|Extra Information:||Star Forming Regions,
Proceedings of IAU Symposium No 115, held 11-15 November 1985 in Tokyo, Japan.
Edited by M. Peimbert and J. Jugaku.
Dordrecht: D. Reidel Publishing Co., 1987
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||G. J. White|
|Date Deposited:||18 May 2012 09:17|
|Last Modified:||12 Aug 2016 19:24|
|Share this page:|