Copy the page URI to the clipboard
Urquhart, J. S.; Thompson, M. A.; Morgan, L. K. and White, Glenn
(2006).
DOI: https://doi.org/10.1017/s1743921307002712
Abstract
We present the results of a multi-wavelength line and continuum study of the brightrimmed cloud SFO 75 in an attempt to determine whether the ionisation front and its associated shocks, driven by the nearby O star, have riggered the formation of a new generation of stars
within this bright-rimmed cloud.
Viewing alternatives
Metrics
Public Attention
Altmetrics from AltmetricNumber of Citations
Citations from Dimensions- Published Version (PDF) This file is not available for public download
Item Actions
Export
About
- Item ORO ID
- 24779
- Item Type
- Journal Item
- ISSN
- 1743-9221
- Keywords
- radio continuum:stars; stars:formation; stars: pre-main sequence
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Copyright Holders
- © 2007 International Astronomical Union
- Depositing User
- Tracy Bartlett