Chemical Abundance Analysis of Population II Stars : The Summary Includes a Background in General Astronomy

Chemical Abundance Analysis of Population II Stars : The Summary Includes a Background in General Astronomy

We are made of stardust in the sense that most atomic nuclei around us have been formed by stars. Stars synthesise new elements and expel them to the interstellar medium, from which later new generations of stars are born. We can map this chemical evolution by analysing the atmospheric contents of o...

Full description

Bibliographic Details
Main Author: Jonsell, Karin
Format: Doctoral Thesis
Language:English
Published: Uppsala universitet, Institutionen för astronomi och rymdfysik 2005
Subjects:
Astronomy
Galactic evolution
Halo
Milky Way
Oxygen
r-element
s-element
Stellar abundances
Astronomi
Astronomy and astrophysics
Astronomi och astrofysik
Online Access:http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-6034
http://nbn-resolving.de/urn:isbn:91-554-6382-7

Internet

http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-6034
http://nbn-resolving.de/urn:isbn:91-554-6382-7

Similar Items