Dolan, J. J. (2016) Probing the Kinematic Structure of Massive core with Molecular lines. Master's Thesis / Essay, Astronomy.
|
Text
Masters_thesis_FINAL24June2016.pdf - Published Version Download (7MB) | Preview |
|
Text
Toestemming.pdf - Other Restricted to Backend only Download (376kB) |
Abstract
The earliest stages of high mass star formation are not very well understood. ”Infrared Dark Clouds” (IRDCs) are a promising candidate for the potential birthplaces of massive stars. By observing molecular lines in these clouds, we can build a picture of the chemical and dynamical structure of the embedded cores in these clouds and study the early stages of high mass star formation.
Item Type: | Thesis (Master's Thesis / Essay) |
---|---|
Degree programme: | Astronomy |
Thesis type: | Master's Thesis / Essay |
Language: | English |
Date Deposited: | 15 Feb 2018 08:13 |
Last Modified: | 15 Feb 2018 08:13 |
URI: | https://fse.studenttheses.ub.rug.nl/id/eprint/14143 |
Actions (login required)
View Item |