Tothill, N. F. H. and White, Glenn J.
(2000).
|
Due to copyright restrictions, this file is not available for public download |
| URL: | http://adsabs.harvard.edu/full/2000ASPC..217..173T |
|---|---|
| Google Scholar: | Look up in Google Scholar |
Abstract
The Lagoon Nebula, M8, has been mapped at 450 μm, 850 μm, and 1.3 mm, using SCUBA and the IRAM 30-m telescope. The large-scale maps (~20' × 10') show clumpy structures surrounding the H II region, extending as far as M8E. The core sizes are around 15" - 30" (0.1 - 0.3 pc), with temperatures of 10 - 40 K. The mass spectrum of the cores is derived, together with estimates of the likely errors. The problems of measuring cores in regions of high-mass star formation are noted.
| Item Type: | Conference or Workshop Item |
|---|---|
| Copyright Holders: | 2000 Astronomical Society of the Pacific |
| Academic Unit/School: | 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) |
| Related URLs: | |
| Item ID: | 32661 |
| Depositing User: | G. J. White |
| Date Deposited: | 23 Feb 2012 16:55 |
| Last Modified: | 29 Nov 2016 22:00 |
| URI: | http://oro.open.ac.uk/id/eprint/32661 |
| Share this page: |     |