Undersökning av döende stjärnor: Massförlust och molekyler för stjärnor på den asymptotiska jättegrenen
dc.contributor.author | Gustafsson, Johan | |
dc.contributor.author | Hirvonen, Per | |
dc.contributor.author | Strömfors, Amanda | |
dc.contributor.author | Wäpling, Sara | |
dc.contributor.department | Chalmers tekniska högskola / Institutionen för rymd-, geo- och miljövetenskap | sv |
dc.contributor.department | Chalmers University of Technology / Department of Space, Earth and Environment | en |
dc.date.accessioned | 2019-07-05T11:52:44Z | |
dc.date.available | 2019-07-05T11:52:44Z | |
dc.date.issued | 2019 | |
dc.description.abstract | The study aims to investigate the mass outflow from evolved stars. Emission lines from nine stars, observed under the project DEATHSTAR, were studied. The gasmass- loss rates were approximated using a simplified formula based on the rotational emission lines of 12CO. Furthermore, the project aims to determine the molecular composition of two of the nine stars, W Hya and R For. The calculated gas-mass-loss rates varied from 10−7 to 10−5M yr−1. The dust-mass and dust-mass-loss rate calculations were only attempted regarding the star W Hya, though no dust-mass and dust-mass-loss could be determined from the data. The observed emission spectra from W Hya and R For contained at least 16 and 17 molecular emission lines respectively. The outflow of W Hya is dominated by oxygen based molecules, while the outflow of R For contains carbon based molecules. Finally, the emission lines from 12CO for several stars show evidence of asymmetric envelopes. The obtained profile for R Hya hints at multiple velocity components and might warrant a more in-depth investigation in the future. | |
dc.identifier.uri | https://hdl.handle.net/20.500.12380/256820 | |
dc.language.iso | swe | |
dc.setspec.uppsok | Technology | |
dc.subject | Fysik | |
dc.subject | Astronomi, astrofysik och kosmologi | |
dc.subject | Physical Sciences | |
dc.subject | Astronomy, Astrophysics and Cosmology | |
dc.title | Undersökning av döende stjärnor: Massförlust och molekyler för stjärnor på den asymptotiska jättegrenen | |
dc.type.degree | Examensarbete för kandidatexamen | sv |
dc.type.degree | Bachelor Thesis | en |
dc.type.uppsok | M2 |
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