Dynamical atmospheres and winds of M-type AGB stars
Mass loss, in the form of slow stellar winds, is a decisive factor for the evolution of cool luminous giants, eventually turning them into white dwarfs. These dense outflows are also a key factor in the enrichment of the interstellar medium with newly produced elements from the interior of these sta...
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| Format: | Doctoral Thesis |
| Language: | English |
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Uppsala universitet, Institutionen för fysik och astronomi
2014
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| Online Access: | http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-230645 http://nbn-resolving.de/urn:isbn:978-91-554-9015-7 |